The galaxy presents as a centrally concentrated, relatively smooth, and slightly elongated object. The core appears to be a bright, unresolved central bulge with a golden hue, suggesting an older stellar population. There is no strong evidence of spiral arm structures or distinct features such as dust lanes or prominent HII regions. The galaxy appears to be relatively isolated, showing no strong tidal features or morphological disturbances indicative of a recent major merger event, although subtle disturbances cannot be ruled out. The overall morphology suggests a galaxy that is either an elliptical galaxy or a lenticular galaxy viewed close to face-on. The color gradient from the core to the outer regions suggests a radial distribution of stellar populations, with potentially younger, bluer stars in the outer disk region. The galaxy appears to have a moderate size.
