The galaxy presents as a relatively smooth, elliptical-like structure. It appears to be generally rounded in shape, with a bright, concentrated central bulge. Faint, diffuse extensions of light are visible extending outwards from the central region. There is a suggestion of a disk-like feature, albeit poorly defined. No distinct spiral arms or strong dust lanes are discernible. The color profile suggests a population of older stars, with a yellowish hue dominating the central regions, transitioning to slightly bluer tones in the outer regions, possibly indicating some ongoing or recent star formation. Overall, the galaxy exhibits characteristics consistent with a transitional morphological type, possibly between a pure elliptical and a lenticular galaxy.
