The galaxy presents an overall elongated, cigar-shaped morphology. The central region appears relatively smooth and concentrated, exhibiting a yellowish-red hue, suggesting an older stellar population. Moving outward from the core, there is a gradual decrease in surface brightness. The outer regions exhibit a bluer tint, potentially indicative of younger stars or ongoing star formation. Faint, diffuse extensions are observed at the extremities, hinting at tidal interactions or past merger events. There is no clear evidence of spiral arm structure, though there is some unevenness in the structure, which could signify some disturbances.