The galaxy presents as a slightly elongated, diffuse object. It exhibits a centrally concentrated light profile, with a smooth, gradual decrease in brightness towards its outer edges. There are no distinct spiral arms or bar structures visible. The color appears predominantly yellowish-white, suggesting a stellar population that is neither overwhelmingly young and blue, nor extremely old and red, but rather a mix that leans slightly older. The smoothness of the light distribution indicates it is most likely an elliptical galaxy, possibly an S0 type, based on the shape. There is no obvious evidence of ongoing major mergers or tidal disturbances, although minor disturbances cannot be ruled out. The estimated size suggests it's a relatively large galaxy.
