The galaxy presents as a relatively smooth, disk-shaped structure viewed at an oblique angle. It exhibits a pronounced central bulge that is bright yellow, indicating a high concentration of older stars. The disk is a fainter, whiter color than the central bulge, suggesting the presence of a younger stellar population and some ongoing star formation. It appears that there are no well-defined spiral arms, and the edges are smooth, indicating that it's a fairly evolved galaxy, with low current star-formation rates.

The overall morphology is most likely that of a lenticular galaxy. There is a slight elongation, as opposed to a perfect circle, making it fall somewhere between a round and a cigar shape. I see very little evidence of dust lanes or recent mergers; there are no obvious tidal tails or other visual disturbances. Overall, it's a pretty uniform, undistributed galaxy that appears to be evolving passively.
