The galaxy presents as a somewhat elongated, lenticular-like structure. It appears relatively smooth in texture, lacking prominent spiral arm features. The central bulge is not distinctly pronounced, but there is a subtle concentration of light towards the galactic center. There is possibly the presence of a faint and diffuse disk. The galaxy's color appears to be slightly redder, potentially indicating an older stellar population and less active star formation. There appears to be a minor perturbation or tidal tail on one side of the galaxy, hinting at a possible interaction or past merger event. Overall, the galaxy seems to be a relatively quiescent system with a moderate mass, exhibiting weak star-forming activity.
