The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, decreasing in luminosity outwards. There is a slight elongation to the shape, more of an in-between rounded and cigar-shaped shape. No distinct spiral arms or bar structures are discernible. The color gradient appears consistent across the galaxy, suggesting a relatively homogenous stellar population. Based on the red color, it appears it is composed mostly of older stars. There may be a slight asymmetry or minor disturbance in the outer regions, but no strong evidence of a major merger event or significant tidal features. The galaxy is compact in size, implying a system in a relatively advanced stage of evolution.
