The galaxy presents as an edge-on spiral system, characterized by a prominent central bulge and a flattened disk. The bulge exhibits a smooth, concentrated light profile suggestive of an older stellar population. The surrounding disk appears thin, and it is likely rotating. The galaxy displays a noticeable color gradient, shifting from bluer hues at the periphery to redder tones toward the bulge. This color gradient is consistent with ongoing star formation in the outer regions and an older stellar population concentrated in the bulge. There are no immediately obvious signs of major mergers or significant tidal disturbances, although the presence of subtle irregularities cannot be completely ruled out without higher-resolution imaging. Overall, the morphology suggests a relatively quiescent, disk-dominated galaxy.
