The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. Its overall shape is somewhat elongated, but not highly cigar-shaped. The galaxy has a yellow-orange color, suggesting a population of older stars with a low rate of on-going star formation. There is no discernible evidence of spiral arm structure or a prominent disk component. The light is centrally concentrated, with a smooth decrease in brightness towards the outer edges. No signs of major mergers or tidal disturbances are visible; it appears undisturbed.
