The galaxy exhibits an elliptical morphology, appearing largely smooth with a high degree of central concentration. The light profile suggests a spheroidal structure with a prominent bulge. There is no discernible spiral arm structure or obvious dust lane obscuration present in the visible light image. Color gradients indicate the core region is more yellow/white in comparison to the outer regions that are more reddish, possibly indicating an older stellar population within the core. The overall appearance is consistent with an early-type galaxy. The galaxy appears to be relatively isolated with no obvious signs of tidal disturbances or ongoing interactions with nearby galaxies.
