This galaxy appears to be a relatively smooth, centrally concentrated system. The light distribution suggests an elliptical morphology, with a notable lack of spiral arm structure or prominent dust lanes. The core region exhibits a bright, yellowish hue that gradually fades into a redder periphery. While the bulk of the galaxy appears featureless, there might be slight indications of minor disturbances or tidal features at the outskirts, but these are subtle. The overall roundness of the galaxy suggests a classification towards the E0-E3 range on the Hubble sequence. The estimated size of the galaxy indicates a substantial physical extent. Star formation rate appears to be low, with a resultant low specific star formation rate, which could be indicative of a more evolved system.
