The galaxy presents as a concentrated, elliptical-like structure. The central bulge exhibits a bright, yellowish-orange hue, suggesting an older stellar population. There appears to be a gradual decrease in surface brightness extending outwards from the core. Some disk like features may be present. There is a faint blue color in areas just outside the center, suggestive of active star formation. The overall structure appears relatively undisturbed, lacking any obvious signs of a recent major merger. Faint wisps and irregularities may indicate minor tidal interactions or internal processes.
