The galaxy presents as a relatively smooth, elliptical-like structure. There appears to be a centrally concentrated bulge, with a gradual decrease in luminosity outward from the center. The galaxy exhibits a yellowish hue, possibly indicative of an older stellar population with lower rates of recent star formation. There are no obvious spiral arms or prominent dust lanes visible. There are no indications of any major mergers or tidal disturbances present in the image.
