The galaxy presents as a centrally concentrated, somewhat elliptical object. It exhibits a smooth, diffuse morphology, lacking prominent spiral arms or a distinct bulge. The central region appears very bright, suggesting a high concentration of stars or possibly an active galactic nucleus, though no distinct point source is visible. The outer regions gradually fade into the background, with a relatively smooth transition, which may indicate a well-mixed stellar population. There is a slight color gradient, with the central region appearing slightly bluer compared to the more reddish outer edges of the galaxy, which could signify the potential presence of some ongoing star formation in the core. Overall, this appears to be a relatively evolved galaxy.
