The galaxy presents as a centrally concentrated object with a relatively smooth morphology. The light distribution appears largely elliptical in shape, with a high degree of circularity. There is little evidence of spiral arm structure or prominent dust lanes. The galaxy exhibits a color gradient, appearing more yellowish-white towards the center, suggesting an older stellar population concentrated in the core. The outer regions exhibit a bluer hue, although this is less pronounced, potentially indicating the presence of younger stars, but at a low rate of star formation. There is minimal distortion or asymmetry, implying it has likely not undergone a recent major merger event. Faint tidal features are absent, indicating a lack of significant gravitational interaction with other nearby galaxies. The overall appearance is consistent with a massive galaxy, with a relatively high mass estimate and low star formation rate.
