This galaxy appears to be a relatively smooth, elliptical galaxy, with a dominant central bulge. The light profile suggests a high degree of symmetry. There is no visible spiral arm structure or significant dust lane obscuration. The color indices indicate a population of older stars, as evidenced by its reddish hue, typical of early-type galaxies. The isophotes appear generally round, although there may be a slight elongation along one axis. There is no obvious evidence of recent or ongoing mergers or tidal interactions with other galaxies, nor is there a distinct active galactic nucleus. The galaxy appears to be relatively quiescent in terms of star formation activity.
