The galaxy presents a somewhat elongated, cigar-shaped morphology. The central bulge region exhibits a concentrated, bright luminosity, displaying a yellowish-white hue, suggestive of an older stellar population. Extending outwards from the core, a fainter, diffuse disk component appears, tinted with redder tones, possibly indicating the presence of dust lanes or regions of on-going, but reduced, star formation. The galaxy shows no visually discernible spiral arm structure. There appears to be a faint, bluish area on one side of the main body, suggesting some recent star formation. Overall the object does not present a highly disturbed morphology, but hints of minor tidal features cannot be fully ruled out at this resolution.
