This galaxy appears to be an elliptical galaxy, exhibiting a smooth, concentrated light profile. Its shape is somewhat elongated, suggesting a possible transition between a more spherical and a disk-like morphology. There may be a slight disk. The galaxy's central region is considerably brighter than its outer regions, indicating a concentration of stars toward the core. There is no strong presence of spiral arm structure or prominent dust lanes, further supporting its classification as an elliptical galaxy. The color appears slightly redder, suggesting a population of older stars. There are no obvious signs of any major merger activity, such as tidal tails or distorted shapes.
