The galaxy presents as a lenticular or early-type spiral, with a prominent central bulge that appears to be composed of older stars, indicated by its yellowish-white color. A faint, disklike structure surrounds the bulge, exhibiting a bluer tint suggesting ongoing or recent star formation. The disk is not clearly resolved into spiral arms but seems to possess some degree of organized structure. The object is moderately elongated with a relatively smooth appearance, although there are indications of possible minor disturbance within the disc. Overall, the galaxy seems to be undergoing relatively low-level star formation, potentially transitioning towards a quiescent phase.
