The galaxy presents as a spiral galaxy viewed nearly edge-on from our line of sight. A prominent central bulge dominates the core region, exhibiting a yellowish hue indicative of an older stellar population. The disk is very thin, and is the main feature that indicates that the galaxy is spiral. This disk appears to be composed of cooler, redder stars. Overall, the galaxy is a smooth, well-defined structure without obvious signs of tidal disturbances or ongoing major merging events. This is likely a stable, relatively undisturbed galaxy.
