The galaxy presents as a single, centrally concentrated object. It exhibits a largely smooth morphology, lacking prominent spiral arms or a distinct disk structure. The light distribution suggests a spheroid-dominated system, potentially an elliptical galaxy or a lenticular galaxy viewed face-on.

The central region displays a higher surface brightness and a yellowish hue, possibly indicating an older stellar population and lower rates of on-going star formation. The outer regions fade gradually into the background sky. There are no strong indications of tidal features or recent merger activity in the immediate vicinity of the galaxy. The overall shape appears slightly elongated.
