The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. A bright, yellowish core dominates the visual appearance, suggesting a concentration of older stellar populations and potentially a supermassive black hole actively accreting material. Fainter, diffuse light extends outwards from the core, exhibiting a gradual decrease in surface brightness. There is a slight elongation along one axis, hinting at a mild deviation from a perfect sphere. The galaxy exhibits a redder color profile towards the center and slightly bluer hues in the outer regions, hinting at the possible distribution of younger stars. There is no clear evidence of spiral arms, a distinct dust lane, or significant tidal features indicating recent or ongoing major mergers. The object is relatively isolated, and the surrounding field does not seem to show evidence of strong interactions with nearby galaxies.
