The galaxy appears as a single, centrally concentrated object with a smooth, symmetrical morphology. Its light is dominated by a yellowish hue, suggesting a relatively old stellar population. There is no strong evidence of spiral arms or a distinct disk structure. The galaxy exhibits a notable central bulge, possibly indicative of a supermassive black hole at its core. The overall impression is that of an elliptical galaxy with little ongoing star formation and a substantial mass. The galaxy appears relatively isolated, showing no signs of major tidal disruption or ongoing mergers. The light distribution fades gradually from the center outwards.
