The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated morphology. The central region is bright and appears yellowish, possibly indicating an older stellar population. The outer regions fade gradually into the background sky. There may be a slight elongation in the shape of the galaxy, but it is mostly round. There is no prominent disk structure visible, or any indications of spiral arms or dust lanes. There are no obvious signs of any major ongoing mergers or tidal disturbances, although there may be some slight asymmetry hinting at a previous minor interaction.
