The galaxy presents as an elongated, cigar-shaped structure. It displays a smooth, centrally concentrated light distribution with a gradual decrease in surface brightness towards the outer edges. The core exhibits a bright, yellowish-white hue, suggesting an older stellar population. Moving outward from the core, the color becomes slightly bluer, especially at the edges. There is subtle evidence of a disk-like structure, though features are not very distinct. The overall form lacks strong spiral arms. The galaxy appears isolated, with no obvious signs of interaction or tidal disturbances.
