The galaxy appears to be a single, relatively smooth object. It exhibits an elliptical morphology with a high degree of roundness. There is no discernible evidence of spiral arms or a central bar structure. The light distribution suggests a centrally concentrated spheroid.

The galaxy displays a color gradient, appearing more yellow in the central region and slightly redder in the outer regions, possibly indicating an older stellar population or a higher concentration of dust in the core. There is no evidence of major mergers or tidal disturbances, with only a slight possibility of a minor disturbance. Overall, the galaxy appears to be an evolved system with a likely dominant bulge component and little ongoing star formation.
