This galaxy exhibits a generally smooth, elliptical morphology. The light profile appears concentrated toward the center with a gradual decrease in intensity outwards. The color is predominantly yellow/orange, suggesting a stellar population dominated by older stars. There is little evidence of spiral arm structure or significant dust lanes. The object appears relatively undisturbed, showing no signs of major merging activity. The axial ratio suggests a nearly circular form when viewed from our perspective, with a hint of elongation. Overall, the galaxy seems to be a relatively evolved system with low ongoing star formation.
