The galaxy presents as a relatively smooth, concentrated object. The light is dominated by a bright central region, possibly a bulge or active galactic nucleus. There is an extended, fainter halo surrounding the core.

The galaxy appears somewhat elliptical in shape, displaying an intermediate degree of roundness. There is no apparent spiral structure, nor are there signs of any ongoing major merger activity. There is a slight suggestion of minor disturbance or tidal features in the outer regions, but these are not pronounced.

The color gradients suggest a population of older stars and indicate relatively moderate levels of ongoing star formation. The overall color index indicates this galaxy has high luminosity. Its estimated size implies it is a large and massive galaxy.
