The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. It exhibits a yellow-red hue, indicating a population of older stars with less ongoing star formation. The galaxy appears generally round in shape with some indication of disturbances. There is a less dense, dimmer region of light below the center of the galaxy with a similar color profile. Based on color, size, and morphology, this is likely a massive galaxy, potentially containing a supermassive black hole at its center. The low star formation rate suggests that this galaxy has likely exhausted most of its gas supply for stellar birth. The overall morphology points to a galaxy that is not currently undergoing significant merging activity, although there are minor disturbances visible.
