The galaxy appears to be a relatively smooth, elliptical or lenticular system. It exhibits a centrally concentrated bulge with a gradual decrease in luminosity outward. There is a discernible color gradient within the galaxy, with the central region appearing more yellow, suggestive of an older stellar population. The outer regions are a bit redder, but the color differences are not very dramatic. No prominent spiral arms or dust lanes are readily visible. The overall morphology suggests a galaxy that has undergone significant evolution and may be relatively quiescent in terms of star formation. There are no significant distortions or tidal features visible in the image, indicating a lack of recent major merger events. Overall the galaxy appears to be relatively isolated and unperturbed.
