The object appears to be a relatively smooth galaxy, exhibiting a centrally concentrated light distribution. The overall morphology suggests an elliptical or lenticular type galaxy, with a high degree of symmetry. The galaxy presents a yellowish color, potentially indicating an older stellar population and lower levels of ongoing star formation. The galaxy's roundness, lack of discernible disk-like structures, and high degree of smoothness contribute to its classification as a spheroid-dominated system. There is no obvious evidence of strong tidal interactions or recent merger events. Faint extensions of light may be present in the outer regions, although the resolution is limited.
