The galaxy presents as a spiral, viewed at an oblique angle relative to our line of sight. Its overall morphology is characterized by a central bulge exhibiting a smooth, concentrated light distribution that dominates the core. Surrounding the bulge, a disk structure is observed, although the spiral arms appear somewhat tightly wound and less well-defined. There may be a bar structure within the central region, that runs from corner to corner on the image. The light distribution within the disk fades gradually with increasing distance from the bulge, indicating an older stellar population. The galaxy exhibits a modest degree of rotational symmetry.
