The galaxy presents a generally smooth, elliptical morphology. Its light profile exhibits a concentrated bulge region that dominates the overall luminosity. There is little to no evidence of spiral arm structure or a prominent disk component. The galaxy exhibits a color gradient, appearing more yellow towards the central bulge, suggesting an older stellar population concentrated in this region, with slightly bluer hues in the outer regions, which indicates the presence of some young stars but their formation rate is relatively low. The overall form is largely undisturbed, showing no obvious signs of a recent major merger or tidal interaction. There are some small disturbances, but they do not appear to be significant. It is fairly round and the presence of a spheroid is more apparent than that of a flattened disk.
