The galaxy exhibits an elliptical morphology, appearing largely smooth in texture. The light distribution is concentrated towards the center, with a gradual decrease in intensity outward. The core displays a yellowish hue, suggesting a population of older stars. Fainter, bluer regions are observed in the outer portions, potentially indicative of some ongoing star formation. The overall shape is somewhat elongated, but not highly so. There are no obvious signs of strong tidal interactions or major mergers, although there may be some subtle asymmetry suggestive of a minor disturbance.
