The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with the brightest region residing in the core. The galaxy's shape approximates a sphere. There is little evidence of spiral arms or a disk-like structure. Faint, diffuse features are visible surrounding the main body of the galaxy, which may be evidence of minor disturbances. There does not appear to be any clear evidence of on-going merging activity or major tidal disruption. The overall color suggests an older stellar population, typical of elliptical galaxies.
