The galaxy presents as a relatively smooth, elliptical morphology. Its light is concentrated towards the core, exhibiting a centrally bright nucleus, with luminosity decreasing gradually outwards. The galaxy exhibits a color gradient, appearing yellower towards the center, suggesting an older stellar population in the core, and becoming somewhat bluer in the outer regions, which might indicate the presence of younger stars or ongoing star formation, albeit at a low rate. No strong spiral arm structures or prominent dust lanes are visible. There are no obvious signs of major merger activity or significant tidal disturbances in its immediate vicinity. The overall appearance suggests a relatively evolved galaxy with a substantial stellar mass.
