The galaxy appears to be of irregular morphology. At its core is an extremely bright, somewhat circular and very concentrated region exhibiting a dominant blue-white color suggesting a high concentration of young, massive stars and/or a possible active galactic nucleus. This central region is relatively small, approximately 4 arcseconds across, and seems to be surrounded by a faint, diffuse halo of reddish-purple light. The reddish tint of the halo could be due to a population of older stars or dust obscuration. There is a possibility of some minor tidal disturbance, with faint wisps or extensions emerging at the top of the galaxy. The overall structure hints at a potentially ongoing or recent merger event, although the primary body of the galaxy seems relatively intact despite the central activity.
