The galaxy appears as a centrally concentrated object with a moderately elliptical morphology. The light distribution is relatively smooth and diffuse, suggesting a lack of prominent spiral arms or distinct substructures. The color gradient indicates a redder core region, potentially indicative of an older stellar population, surrounded by a bluer, more extended halo. The overall appearance is consistent with an early-type galaxy, potentially an elliptical or lenticular system exhibiting ongoing or recent star formation. The absence of clear tidal features suggests it is not undergoing a major merger, although some minor disturbances may be present. The galaxy appears to have a large, fuzzy disk.
