The galaxy presents as a centrally concentrated, smooth system with a generally elliptical morphology, observed with a possible slight inclination. The core region is bright and appears to be dominated by an older stellar population, exhibiting a yellow-red hue indicative of evolved stars. There is a subtle disk component. The outer regions of the galaxy show fainter, bluer colors, suggesting ongoing or recent star formation, although at a relatively low rate. There is no apparent ongoing merger activity or strong tidal features detected in the image. The overall structure appears relatively undisturbed.
