The galaxy presents as a lenticular or early-type spiral galaxy, seen at a high inclination. It exhibits a generally smooth, elongated morphology. A prominent central bulge is visible, displaying a yellowish hue, suggestive of an older stellar population. There's little to no apparent active star formation within the bulge. Fainter, bluer regions extend from the bulge, potentially indicating the presence of a disk structure containing younger stars and some ongoing star formation, though it is relatively quiescent. There is no visible evidence of a recent major merger event. Minor disturbances cannot be completely ruled out based on the morphology alone. The overall color suggests that the galaxy is relatively evolved, with a dominant population of older stars and a low rate of ongoing star formation.
