The galaxy presents a smooth, elongated morphology, appearing cigar-shaped. Its central region exhibits a yellowish hue, suggesting a population of older stars. Proceeding outwards from the center, the color seems to transition to a bluer color indicating presence of younger stars. There is no indication of a prominent spiral structure or significant dust lanes from what is visible. There is little evidence of any major disturbances or ongoing mergers; it appears to be a relatively undisturbed system.
