The galaxy appears to be a roughly elliptical system with a smooth overall structure, though some finer features suggest internal activity. The central region is characterized by a bright, concentrated area, possibly indicative of an active galactic nucleus or a dense stellar population. The galaxy exhibits a color gradient, transitioning from a yellow-orange core to bluer outer regions. This suggests a possible difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars forming in the outskirts. There is some evidence of tidal disturbances. The shape indicates it is not a perfect ellipse and that the galaxy is undergoing interactions.
