The galaxy appears to be a relatively smooth, elongated structure. Its central region exhibits a higher surface brightness with a yellowish hue, suggesting an older stellar population is dominant in this area. The outer regions appear more diffuse with a bluer tint, potentially indicating the presence of younger, hotter stars, and regions of active star formation. The galaxy seems to have a somewhat disturbed morphology, hinting at a possible past interaction or merger, although a major disruption is not readily apparent. There is a slight asymmetry in the outer regions of the galaxy.
