The galaxy presents as a centrally concentrated object with a smooth overall morphology. It exhibits a roughly elliptical shape, appearing highly rounded. The core region displays a bright, intense glow, suggestive of a dense stellar population and/or possible active galactic nucleus activity, though further spectral analysis would be needed to confirm AGN presence. There is a general color gradient apparent, with the core appearing more yellow/white in color, and the outer regions gradually becoming more red. This could be indicative of an older stellar population in the galaxy's halo and disc, or obscuration. The smooth appearance and concentrated central bulge suggest that this is likely an early-type galaxy, such as an elliptical galaxy or a lenticular galaxy. There may be minor tidal disturbances, or an interaction with another galaxy. The relatively smooth texture is consistent with a lack of active or recent star formation. The general morphology implies it has undergone significant evolution, possibly including past merging events. Further data, including spectroscopic analysis, is necessary for a definitive classification.
