The galaxy appears to be a relatively smooth, elliptical system. The overall shape is elongated, with a cigar-like appearance. There is a central, brighter region that is concentrated and diffuse. Fainter and more diffuse light surrounds this central concentration. The galaxy displays no prominent spiral arm structure or dust lanes. The light is slightly bluer in the central region, suggestive of some star formation activity. The outer regions display redder colors, which indicate an older stellar population. There are no strong signs of any major mergers or significant tidal disturbances, though a minor disturbance cannot be ruled out.
