The galaxy presents as an edge-on disk galaxy with a prominent central bulge. The bulge appears smooth and somewhat elongated along the major axis of the disk. The disk itself exhibits a relatively smooth appearance, with a noticeable thin dust lane that may be indicative of ongoing, albeit low, star formation. The overall color gradient suggests older stellar populations dominating the bulge, while the presence of the dust lane hints at the possibility of younger stars within the disk. The galaxy has a moderate inclination relative to our line of sight, allowing for some structural details to be discernable. The ellipticity of the galaxy appears high, reflecting its edge-on nature. There appears to be no distinct spiral structure, suggesting it may be a lenticular galaxy or a late-type spiral with tightly wound arms that cannot be resolved at this distance. No signs of strong tidal interactions or mergers are readily apparent.
