The galaxy presents as a moderately luminous, disk-shaped system viewed at a slight angle from edge-on. Its central bulge appears bright and concentrated, with a yellowish hue suggesting an older stellar population. The disk itself exhibits a smoother texture with faint arms indicating that it has some spiral structure, but overall appears quite blended. The color gradient transitions from yellow-white in the core to a slightly bluer tinge in the outer disk, possibly indicating younger stars in those regions. Overall, the galaxy does not show strong evidence of active star formation or recent major merger activity, however, the disturbances observed within the image suggest it may have experienced some form of past interaction.
