This galaxy presents an elongated, disk-like morphology, viewed at a considerable angle relative to its plane. A bright, concentrated central bulge is evident, suggesting a relatively substantial spheroidal component. The overall color appears moderately red, indicating a population of older stars. The disk exhibits a faint, diffuse spiral structure, with hints of spiral arms extending outwards from the central bulge. There is a notable asymmetry observed in the outer regions of the disk, potentially indicative of tidal interactions or past merger events. The galaxy appears relatively smooth in texture, with no prominent dust lanes readily apparent in this image.
