The galaxy presents as an edge-on spiral, characterized by a distinct disk-like structure. The central bulge exhibits a smoothly rounded morphology. There are hints of a faint dust lane bisecting the galaxy's mid-plane, although image resolution limits clear delineation. The disk appears relatively smooth, lacking prominent spiral arm structures. The color profile suggests an older stellar population, with a yellow-red hue dominating the galaxy's light emission. There is no evidence of ongoing major mergers or significant tidal disturbances, although very faint and subtle asymmetries may exist. Overall, the galaxy appears to be a relatively undisturbed and well-defined system.
