The galaxy presents a morphology that appears largely elliptical, exhibiting a smooth, diffuse light distribution. The central region is characterized by a concentrated, bright core. The overall shape is somewhere in between round and elliptical. There appears to be minor structural distortion present, possibly indicating an ongoing or past interaction. The galaxy displays a color gradient, with the core appearing yellower compared to the bluer outer regions. This suggests a central population of older stars, surrounded by a younger stellar population. There are hints of faint features which could indicate a disk, but it is difficult to confirm from this image.
