The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. It exhibits a color gradient, with the core appearing more yellow-white, possibly indicative of an older stellar population. The outer regions fade into a bluish hue, suggesting some ongoing, though perhaps subdued, star formation. There is no obvious spiral arm structure or significant dust lane obscuration visible. The galaxy appears relatively isolated, lacking evidence of recent major mergers or tidal disturbances. Overall, this galaxy appears to be a relatively quiescent system, transitioning towards an early-type morphology.
