The galaxy presents as an object of moderate apparent size, approximately circular in projection. It exhibits a centrally concentrated morphology with a bright core region. The overall light distribution appears relatively smooth, although subtle features are possibly present. There is a suggestion of a disk-like component and some irregularities and a bluer color distribution in its outer regions, indicative of ongoing or recent star formation. The galaxy's core is predominantly bright and slightly round. Possible disturbances or minor interactions may be influencing the overall structure of this system, evidenced by some asymmetry. There is a chance of a faint merger occurring. The color indices suggest a higher luminosity in the blue bands than in the red bands. 
