The galaxy presents a somewhat smooth, elongated morphology. The primary color gradient transitions from a blueish-white core region to a more yellow/red outer region. The overall shape is reminiscent of a cigar. There are no obvious signs of spiral arm structure or a prominent central bulge. Some minor asymmetry is present, suggesting possible interactions or recent internal activity. The overall appearance indicates a significant population of older stars, particularly in the outskirts, alongside recent star formation in the core. No apparent major disturbances or signs of a major merger are observed.
