This galaxy presents as a centrally concentrated system with a smooth, diffuse morphology, suggesting characteristics of an elliptical or S0-type galaxy. The core exhibits a bright, yellowish-white hue, potentially indicative of an older stellar population. The outer regions fade into a bluish halo, possibly reflecting a more dispersed distribution of younger stars. There is little apparent dust or spiral structure visible. The overall shape appears generally rounded, with a subtle elongation. Indications of any major merger events or significant tidal disturbances are absent, though some minor asymmetry cannot be ruled out. The galaxy's color profile suggests moderate levels of star formation, but not at a rate strong enough to disrupt its smooth appearance.
