The galaxy presents as a relatively smooth, elliptical-like object. Its core is a bright, concentrated region of yellowish-white light, suggesting a high density of older stars. The light fades gradually outwards from the core, with a small change in hue from yellow to red. There appears to be a faint hint of spiral arms, implying a very weak disk, but they are not well-defined. There is no strong evidence of recent or ongoing major mergers or tidal disruptions within this galaxy from the image alone, although the faint structure may indicate a minor disturbance.
