The galaxy presents a morphology suggestive of a disk galaxy, though with a significant bulge component. It is moderately inclined relative to our line of sight. The central region appears luminous and concentrated, indicative of a high stellar density within the bulge. Surrounding the bulge, we observe a fainter, more diffuse disk. There is the possibility of interactions occurring with this galaxy, due to its disturbed morphology. The outer regions of the galaxy exhibit lower surface brightness, gradually fading into the background sky. Its color indices suggest ongoing star formation. The galaxy exhibits some signs of minor disturbances, such as asymmetry and possible tidal features. It exhibits a relatively smooth appearance, but faint disk features suggest it may not be entirely elliptical.
