This galaxy appears to be an elliptical galaxy with a smooth, concentrated light profile. The color suggests an older stellar population, with a significant amount of redder light, possibly indicating a lack of recent star formation in the central regions. It has a slightly elongated shape. There is evidence of some blue light in the outer regions suggesting some disk or spiral features, potentially indicating ongoing, or recent, minor star formation. There is a slight indication of minor disturbances, but overall it appears to be a fairly relaxed, unperturbed system, likely not currently undergoing a major merger. The galaxy exhibits an overall smoothness, with a minimal presence of distinct features.
