The galaxy presents as a relatively compact, disk-like structure oriented approximately horizontally in the frame. The central region exhibits a higher surface brightness compared to the outer regions, suggesting a concentration of stars or other luminous material. The disk component appears relatively smooth, lacking prominent spiral arms or distinct features within the resolution of the image. There is evidence of a slight disturbance or possible faint tidal feature on the upper and lower edges, indicating a potential past interaction or merger event. The overall color appears as mostly luminous, with the central regions appearing brighter than the outer regions. Based on the observations, this galaxy is potentially undergoing a phase of interaction or minor merging with another galaxy.
