The galaxy presents as a relatively smooth, round object. There is a concentration of light towards the center, suggesting a central bulge or core region. The galaxy has a slightly yellowish hue, possibly indicative of an older stellar population. There does not appear to be a well-defined disk structure or spiral arms. There are no obvious signs of any major ongoing merger or tidal disturbances, although there is a slight asymmetry of light distribution on the periphery of the galaxy. Overall, the galaxy exhibits the characteristics of an elliptical galaxy, or possibly a lenticular galaxy seen close to face-on. The colors appear to be consistent with moderate star formation and a generally massive stellar population.
