The galaxy presents a roughly elliptical morphology with a dominant central bulge. The color profile suggests a relatively older stellar population, particularly concentrated within the core, as indicated by the yellowish-white hue. The presence of fainter, slightly bluer regions surrounding the core indicates a possible disk component. The outer regions exhibit subtle disturbances, suggesting a minor interaction or merging event in the past. Overall, the galaxy appears to be undergoing a relatively quiescent phase of star formation.
