The galaxy presents as a somewhat compact, disk-shaped structure viewed at an oblique angle. There is a slight indication of a central bulge, but it is not prominently defined. The overall color of the galaxy appears to be a yellowish-white, which may suggest a relatively older stellar population dominating the light output. There is some indication of bluer regions, particularly in what might be spiral arm structures on one side, suggestive of ongoing star formation. The disk itself appears relatively smooth, lacking strong evidence of prominent dust lanes or significant clumpy star-forming regions. A minor disturbance can be seen in the structure, possibly from a smaller merging event. The overall impression is of a galaxy that may be in a transitional phase, with some characteristics of both spiral and lenticular galaxies.
