This galaxy exhibits a generally smooth morphology with a slight elongation, suggesting an elliptical or lenticular type. The core region is bright and concentrated, displaying a yellowish hue, indicative of an older stellar population and minimal ongoing star formation. The outer regions gradually fade in intensity, forming a diffuse halo. There is some asymmetry present, potentially a minor tidal disturbance. The galaxy appears relatively isolated, with no obvious signs of a major ongoing merger.
