The galaxy presents a primarily smooth morphology, appearing as an elliptical or lenticular system seen at an oblique angle. It exhibits a moderate ellipticity, leaning towards a cigar-shaped appearance. The central bulge is prominent and exhibits a bright, concentrated luminosity, suggesting a significant population of older stars. Fainter, diffuse light extends from the core, exhibiting a slight gradient in color, transitioning from a yellowish-white center to a bluer hue in the outer regions, potentially indicating some ongoing, albeit limited, star formation. There is little to no evidence of spiral arm structure or significant dust lanes. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Any minor disturbances could be occurring, but with no clear indications.
