The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated core. It exhibits a generally rounded shape, showing little evidence of a disk structure. There may be some minor disturbances or tidal features, but the overall structure is dominated by its smooth, spheroid-like morphology. The light distribution is fairly uniform, with a color gradient suggestive of an older stellar population, likely with minimal ongoing star formation. The galaxy does not appear to be strongly interacting or undergoing a major merger. There's a possibility of a minor merger but not a strong one. The absence of defined spiral arms or distinct dust lanes is consistent with a classification as an elliptical galaxy.
