The galaxy presents a generally smooth morphology with a slight elongation. The light distribution indicates a central concentration with a gradual decline in surface brightness towards the outer regions. A faint, diffuse halo surrounds the brighter central area. There is a hint of a disk or spiral structure, but it appears to be disturbed. The color profile suggests an older stellar population, particularly in the central bulge, which exhibits a yellowish hue. The outer regions appear slightly bluer, indicating the presence of younger stars, possibly due to recent or ongoing star formation. Some minor disturbances or tidal features might be present, though they are not very strong. This could potentially be caused by a past interaction with another galaxy, or ongoing merging.