The galaxy appears to be a relatively smooth, elliptical system with a concentrated central bulge. The light distribution suggests an older stellar population, exhibiting a yellowish-red hue in the central region. Fainter extensions can be observed, and the lack of strong blue light indicates minimal ongoing star formation. There is the suggestion of some mild disturbances in the overall smooth shape. There is a second similar-sized object below the main galaxy which appears similar to the first galaxy.