The galaxy presents as a relatively smooth, lenticular or elliptical galaxy. It exhibits a concentrated central bulge that gradually fades into a diffuse halo. The overall shape appears to be somewhere between round and elongated, with a slight tendency toward ellipticity, but not extremely cigar-shaped. There is little evidence of significant spiral arm structure or strong disk features. The color gradient suggests a population of older stars, with a redder hue in the central region. There is a slight indication of possible minor disturbance, with some subtle asymmetries in the outer regions, but overall the galaxy appears to be relatively undisturbed.
