The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance. Its color profile indicates a relatively evolved stellar population, with a yellowish hue dominating the central region, suggesting a prominence of older, redder stars. The galaxy exhibits a moderately elliptical shape, elongated along one axis. There is no discernible spiral arm structure or evidence of significant dust lanes. Overall, the galaxy appears to be a quiescent system with limited ongoing star formation and likely a high stellar mass. The morphology is consistent with an elliptical galaxy in a relatively isolated environment, showing no strong signs of recent or ongoing mergers. There are subtle irregularities in the outer regions of the galaxy, such as faint extensions, but these are very faint, and it could be tidal debris from a minor disturbance.
