The galaxy presents as a relatively smooth, elliptical structure. It exhibits a bright, concentrated core, possibly indicative of an active galactic nucleus or a high density of stars in the central region. There is a moderate distribution of light extending outward from the core, displaying a slight elongation. The color gradient suggests a stellar population that is predominantly older and redder in the central region, transitioning to somewhat bluer hues in the outer regions. The galaxy appears relatively isolated, with no obvious signs of major interactions or ongoing mergers, though a subtle asymmetry in the outer regions could suggest minor gravitational disturbances. There's a hint of a possible disk-like feature, but it's not sharply defined. Overall, the galaxy appears to be a mid-sized galaxy, displaying features of both elliptical and spiral galaxies.
