The galaxy presents as a somewhat disturbed, disk-like structure with a significant central bulge. It exhibits a relatively smooth appearance overall, but with possible minor tidal disturbances. The shape is more in-between than either fully round or cigar-shaped. The disk shows a blue hue, suggestive of ongoing star formation. A brighter, slightly yellowish central region is present, indicative of an older stellar population. The galaxy appears to be undergoing a minor disturbance possibly due to a past interaction.
