The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a predominantly elliptical morphology with a moderate degree of roundness. The central bulge appears prominent and luminous, with a yellowish hue, potentially indicative of an older stellar population. There is a subtle color gradient extending outward from the core, fading into a redder and less luminous halo. No distinct spiral arm structures are visible. There is a slight asymmetry to the outer edges of the halo. The overall appearance suggests that this galaxy is not actively undergoing a major merging event, but minor disturbances may be present.
