The galaxy presents as a relatively smooth, elongated object. The central bulge appears bright and somewhat diffuse, with a yellowish-white hue, suggestive of an older stellar population. Moving outwards from the core, the galaxy appears to gradually fade, transitioning to a fainter bluish-white disk. The disk exhibits minimal apparent structure, with no distinct spiral arms or prominent dust lanes visible at this resolution. The overall morphology leans towards a lenticular or an early-type spiral galaxy, lacking the well-defined features of a late-type spiral. The color profile indicates a potential decline in recent star formation activity. The shape seems to resemble a cigar. No signs of ongoing major mergers or significant tidal disturbances are observed.
