The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light profile. The core region is notably bright and appears yellowish, suggesting a population of older stars dominating the central area. Moving outwards from the center, the luminosity decreases, and the color shifts subtly towards a bluer hue. This might indicate the presence of a younger stellar population in the outer regions, although the overall color remains relatively red. There's a slight elongation observed, with the galaxy appearing more cigar-shaped than perfectly round. There are hints of faint, extended structure, but no strong evidence of spiral arms or significant disturbances indicative of recent major merger events. Some minor asymmetry may be present but any determination beyond this would be speculative.
