The galaxy presents as an elongated, lenticular-like structure. It exhibits a smooth, concentrated bulge that transitions into a flattened disk. There appears to be a lack of distinct spiral arm structures; the disk presents as relatively featureless. Light distribution shows a concentration towards the center, the bulge emitting a more yellowish hue, potentially indicating an older stellar population. The outer regions of the disk appear fainter and exhibit a slightly bluer color profile than the bulge, indicative of younger stars. Overall, the galaxy appears to be in a relatively quiescent state, with little to no signs of active star formation discernible from the image. The galaxy is most likely an edge on spiral galaxy. No signs of tidal disruption, shells, or interacting companions are evident.
