The galaxy appears to be a relatively small, faint object. It exhibits a flattened, disk-like morphology, viewed nearly edge-on from our line of sight. There appears to be a central bulge region that is brighter than the rest of the disk. There is minimal evidence of spiral arm structure. There is a slight asymmetry, possibly indicating a minor tidal interaction or disturbance. The galaxy appears relatively smooth, lacking prominent features. The color is generally redder than the surrounding objects, which suggests a population of older stars or a significant amount of dust obscuring younger, bluer stars. There is not strong evidence to suggest that this galaxy is undergoing a major merging event.
