The galaxy appears to be a relatively smooth, elliptical-like object. It presents a concentrated central bulge which transitions smoothly into a fainter, more diffuse halo. The light is dominated by redder wavelengths. There is no clear spiral arm structure. The shape is generally round but with some slight elongation. There is no evidence of any tidal features or major interactions. The overall morphology is undisturbed, suggesting the galaxy is not currently undergoing any significant merging activity. The star formation rate appears low, consistent with a more evolved stellar population.
