The galaxy presents a largely featureless, smooth morphology, indicative of an elliptical galaxy or a lenticular galaxy viewed face-on. It exhibits a centrally concentrated luminosity profile, peaking in a bright, yellowish core, suggesting an older stellar population dominating the central region. The overall shape is close to circular, showing minimal elongation or asymmetry. There is no clear evidence of spiral arms, bars, or significant dust lanes. The outer regions gradually fade in intensity, displaying a redder hue compared to the core, possibly signifying a gradual decline in star formation activity and the presence of older, redder stars in the galaxy's outskirts. No signs of major ongoing merger activity or tidal disturbances are apparent. The galaxy's relatively compact size and high central concentration imply it is a massive galaxy with a significant stellar mass.
