The galaxy presents a largely smooth, elliptical morphology. The light distribution appears concentrated toward the center, with a gradual falloff in intensity outwards. There is some slight evidence of an asymmetrical feature along one edge, possibly indicating a minor interaction or disturbance. The color profile is largely homogenous with some hint of blue light suggesting some star formation, although this may be older stars. Based on its overall structure and color, this galaxy is likely a moderate to high mass system that is at the end of the blue sequence that has shifted to the red sequence.
