This galaxy appears to be a lenticular or edge-on spiral galaxy. It exhibits a flattened, elongated shape, suggesting that we are observing it nearly edge-on from our vantage point. The central bulge is prominent and appears relatively smooth and featureless. A faint, diffuse disk surrounds the bulge. The disk is slightly bluer in color compared to the bulge, which may indicate the presence of younger stars and ongoing star formation, albeit at a low rate. There is no apparent evidence of active galactic nuclei activity, or significant dust lanes or strong spiral arm structures. There does not appear to be any obvious interaction or merging events occurring. The galaxy appears to be relatively isolated and undisturbed. Overall, it seems to be a quiescent galaxy with a relatively small stellar mass.
