The galaxy appears to be a relatively smooth, early-type galaxy, likely an elliptical. It exhibits a concentrated light profile with no discernible spiral arm structure or significant dust lanes. The object presents with a slightly elongated morphology, not perfectly spherical, but leaning towards a more flattened shape. There are some indications of minor disturbances, such as slight asymmetries in the light distribution, but these do not suggest a major ongoing merger. The galaxy's color suggests a population of older stars. Overall, the light is dominated by reddish tones, with a smaller contribution from bluer wavelengths. This implies that the galaxy has a relatively low rate of ongoing star formation.
