The galaxy presents as a centrally concentrated object with a smooth, symmetrical morphology. The light profile appears elliptical, lacking prominent spiral arms or a distinct disk structure. The core exhibits a yellow-white hue, indicative of an older stellar population. The color shifts gradually outward to a more reddish-orange tint in the outer regions, suggesting further aging of stars away from the center. There is no obvious dust lane or active star forming region visible. The overall appearance points towards a relatively evolved galaxy, potentially an elliptical galaxy or a lenticular galaxy viewed face-on. Slight irregularity appears on the bottom left side, a possible indicator of tidal interactions, merger activity, or distortion.
