The galaxy presents as a relatively smooth, disk-like structure. It is elongated, with a cigar-shaped appearance. The central region exhibits a bright, concentrated core, potentially indicative of a significant stellar population or an active galactic nucleus. The disk shows a subtle color gradient, transitioning from a more reddish hue in the center to a slightly bluer tint in the outer regions. This color variation may suggest differing stellar populations, with older, redder stars concentrated centrally, and younger, bluer stars populating the outer disk, though dust obscuration could also play a role. There is no obvious evidence of strong spiral arm structure or major merger activity. Subtle irregularities in the outer disk suggest possible minor disturbances or interactions.
