The galaxy presents as a fairly smooth and centrally concentrated object. It exhibits a roughly elliptical morphology, appearing neither perfectly spherical nor highly elongated. There is no discernible spiral arm structure or prominent bar feature. The galaxy exhibits a relatively compact core region. Color gradients are subtle but visible, with a slightly bluer hue towards the central regions and a gradual shift to redder tones in the outer regions. No strong signs of recent or ongoing major mergers are readily apparent, although some minor morphological disturbances cannot be ruled out. The overall light distribution suggests a relatively mature stellar population, with some evidence of recent star formation activity in the central regions.
