The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with a subtle elongation. The color profile suggests a higher concentration of older stars towards the center, indicated by the yellowish hue in the core. There is minimal evidence of spiral arm structure or significant dust lanes. The overall light distribution appears diffuse, implying a well-mixed stellar population. Slight asymmetry may be present, suggesting a possible past interaction or minor disturbance but is generally unperturbed.
