The galaxy presents an elliptical morphology, exhibiting a centrally concentrated bulge that dominates the overall light profile. The galaxy appears relatively smooth in texture, with no obvious spiral arm structures. The orientation of the galaxy suggests it is viewed at a significant angle relative to its equatorial plane, presenting an elongated profile on the sky. The color gradient indicates a generally older stellar population throughout the galactic body. The presence of a central bulge suggests the existence of a supermassive black hole. The outer regions of the galaxy appear fainter, consistent with a decreasing stellar density as distance from the center increases. The galaxy appears isolated in its immediate environment, with no obvious signs of tidal interactions or ongoing mergers.
