The galaxy presents as a moderately inclined, disk-like system. The central bulge region appears significant in size and exhibits a smoother, more concentrated light profile, with a yellowish-white hue suggesting an older stellar population. Moving outward from the bulge, a flattened disk is observed, displaying faint spiral arm structures. These arms appear somewhat diffuse and patchy, exhibiting regions of bluer light indicative of ongoing star formation. The overall morphology suggests a possible intermediate spiral type, transitioning from a more bulge-dominated galaxy to a developed spiral. The galaxy shows some minor irregularities in its disk, potentially indicative of a minor gravitational interaction or past merger event, but the overall structure appears relatively undisturbed. The extent of the galaxy is moderate, appearing neither extremely compact nor significantly dispersed. There's a hint of dust lane absorption along the near side of the disk, partially obscuring some of the light from the bulge.
