The galaxy presents as a moderately luminous object with a notable disk-like structure. The central bulge is subtly visible, appearing slightly brighter and more concentrated than the outer regions. The overall color appears somewhat reddish, potentially indicating an older stellar population or a higher dust content within the galaxy. There is some indication of minor disturbances in the galaxy’s structure, perhaps suggesting a past interaction or a minor merger event. The morphology seems to lean towards an intermediate type between a pure elliptical and a spiral, possibly a lenticular galaxy, but with slight irregularities. The galaxy does not appear to be undergoing a major merging event at the current time.
