The galaxy presents as a flattened, disk-shaped structure, viewed at a significant inclination. It appears to have a prominent central bulge, bright and yellowish-white in color, which diminishes in intensity towards the outer regions of the galaxy. The disk exhibits some granularity but lacks a distinctly resolved spiral arm structure in the available image. A subtle bluer component is visible within the outer disk, indicative of a younger stellar population possibly. There is no immediately apparent evidence of major mergers or tidal disturbances. Based on the color gradient from the center to the outer regions, and lack of distinct spiral arms, it may be an intermediate spiral or lenticular galaxy.
