The galaxy appears to be an elliptical galaxy, characterized by a smooth, spheroidal morphology. The light distribution shows a concentration towards the center, with a gradual decrease in brightness towards the outer regions. There is no evidence of spiral arms or a distinct disk structure. The galaxy exhibits a yellowish hue throughout, indicating a population of older stars with fewer young, blue stars. The overall shape is somewhat rounded, although there is a slight elongation suggesting it is not perfectly spherical. No significant signs of ongoing mergers or major disturbances are observed within the galaxy's structure, though there is a subtle asymmetry, which might denote a past interaction. The galaxy appears relatively isolated, without prominent tidal features or nearby interacting galaxies.
