The galaxy presents as an elliptical morphology, exhibiting a smooth, centralized concentration of light. The central bulge appears bright and yellowish-orange, indicating a likely older stellar population. There is a slight elongation observed, transitioning from round to a more cigar-like shape. Evidence for a disk structure is not prominent. No distinct spiral arms or bar features are visible. The galaxy appears relatively undisturbed, showing no signs of major mergers or significant tidal disruptions. There is a possibility of a minor disturbance present, but it is not readily apparent in the image. Overall, the galaxy is an elliptical system with a relatively high mass and low star formation rate.
