The galaxy presents a lenticular morphology, appearing as a flattened, elongated structure with a smooth, diffuse light distribution. There is a slight central bulge but no distinct spiral arm structure visible in this image. The color gradient suggests that the galaxy is slightly bluer in its outer regions, indicating regions of ongoing star formation. The overall color is relatively red, suggesting an older stellar population dominates, consistent with a galaxy that is no longer actively forming many stars. The galaxy appears relatively isolated with no obvious tidal features or close companion galaxies indicating recent or ongoing major mergers, although there may be minor distortions or disturbances present. The galaxy appears fairly massive.
