This galaxy exhibits a moderately elliptical morphology. The light distribution is dominated by a smooth, centrally concentrated component, suggesting a significant spheroidal population of stars. There is a subtle color gradient, with the central region displaying a yellowish hue, potentially indicative of an older stellar population. Fainter blue colors are seen on the outskirts of the galaxy, possibly due to the presence of younger stars. The galaxy shows some low level disturbances to its symmetry, possibly indicative of a past merger event. The central region is relatively compact, while the outer regions extend to a larger diameter.
