The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a subtle elongation, indicating a deviation from a perfectly circular morphology. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population dominating the central regions. Moving outwards from the core, the light gradually fades into a less intense, somewhat reddish halo. Faint disk-like features may be present, but the smooth nature of the galaxy dominates. There is no strong evidence of active star formation regions or spiral arm structures. The galaxy appears relatively undisturbed, with no major signs of recent merger events or significant tidal distortions. Overall, the galaxy seems to be an evolved system with characteristics of a lenticular or early-type spiral galaxy.
