The galaxy appears to be a spiral galaxy, viewed at a near edge-on angle. A distinct bulge is not readily apparent. The visible structure exhibits a relatively smooth, diffuse disk-like appearance, with a somewhat asymmetric distribution of light. There is evidence of a possible tidal tail or a disrupted arm extending from one side of the disk, suggesting a potential past interaction or merger event. Patches of bluer light are observable within the galaxy, likely indicating regions of active star formation. There may be some dust lanes visible but they do not appear very prominent. The overall color of the galaxy has some differences in color, ranging from bluer hues at the edge to more red color. The overall structure is relatively smooth, with indications of disturbance or interaction.
