The galaxy presents as an elongated, relatively smooth structure. The central region exhibits a brighter, more concentrated luminosity, potentially indicative of a bulge. There is a slight color gradient, with the central region appearing somewhat redder compared to the outer edges, which show a bluer hue. This could suggest differing stellar populations, with older stars concentrated in the bulge and younger stars populating the disk. There may be some minor disturbances visible, or it is possibly undergoing a merger. The overall shape appears to be intermediate between round and cigar-shaped. Although the structure is largely smooth, a faint, disk-like component may be present with some arm-like features. The galaxy is observed to have a relatively low star formation rate.
