The galaxy exhibits an irregular morphology with a somewhat clumpy appearance. A central, bright core region is prominent, possibly indicating a concentration of stars and/or an active galactic nucleus. The light distribution surrounding the core is asymmetric. There is some indication of tidal features, suggesting the possibility of an ongoing or past interaction/merger with another galaxy. The galaxy exhibits a faint, diffuse halo, possibly due to stripped stellar material from the interaction. The color distribution is also irregular, which may correspond to different stellar populations across the galaxy.
