The galaxy exhibits a distinct disk morphology, though its orientation is not precisely edge-on. Spiral arm structures are apparent within the disk, although they are not sharply defined. The central bulge is moderately sized, displaying a yellowish hue indicative of an older stellar population. The disk shows bluer regions, suggestive of ongoing star formation. There appear to be some tidal disturbances or minor interactions, though not obviously a major merger. Overall, the galaxy presents a mix of features indicating both established stellar populations and active star forming regions.
