The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that appears yellowish-orange in color, suggestive of an older stellar population. The light is more concentrated at the center of the galaxy with a falloff in intensity at the edge of the galaxy.

Surrounding this core is a fainter, more diffuse halo with a slight blue tint. This halo extends further from the center than the core and is not perfectly circular, appearing slightly elongated. The galaxy does not present any strong spiral arm structures or distinct features, such as dust lanes.

There is no indication of a major ongoing merger, however, subtle asymmetries in the outer regions suggest possible minor gravitational interactions.

Based on its morphology, color, and lack of distinctive features, this galaxy is likely an elliptical galaxy with a relatively low star formation rate.
