The galaxy presents a flattened, elongated morphology, likely indicative of a disk galaxy viewed at a high inclination. The central region exhibits a concentrated bulge, appearing somewhat brighter and more yellow/orange in color, possibly suggesting a population of older stars. Fainter, bluer light extends outwards from the central bulge along the major axis, implying the presence of younger stars and ongoing star formation within the disk. The disk appears relatively smooth. The overall form exhibits a cigar shape, and there is no evidence of spiral arm structure. The galaxy shows no obvious signs of a major merger, although there could be evidence of minor disturbances.
