This galaxy presents as a spiral type, viewed at an angle that is slightly tilted but still permits discernible observation of its disk structure. Distinct, well-defined spiral arms are visible, tracing out from the central bulge region. These arms seem to have an almost "grand design" style.

The central bulge appears moderately sized. There is a concentrated area of light, suggesting older stellar populations towards the core, although its exact morphology is difficult to ascertain from the image alone. No obvious bar structure is observed bisecting the bulge.

The spiral arms exhibit a range of morphologies. Some arms appear tightly wound closer to the central region, while others extend further and are more loosely defined. Patches of bluer light, scattered throughout the disk, hinting at regions of active star formation. The overall color gradient indicates a mixture of stellar populations, with regions of both young, hot stars and older, cooler stars.

There may be signs of mild tidal features or asymmetries in the outer disk, hinting at possible interactions with other galaxies in the past. However, the morphology is predominately characterized by an unperturbed disk. The galaxy overall has a disk dominated morphology, and it's shape is largely dictated by the spiral arms.
