The galaxy presents as a somewhat elongated, cigar-shaped structure. A smooth, centrally concentrated bulge dominates the morphology, exhibiting a yellow-orange hue. The outer regions of the galaxy, moving towards the edges, fade gradually into a faint disk. There is a hint of a greenish tint on one side of the disk, indicating a possible variation in stellar populations or dust content. No distinct spiral arms or prominent dust lanes are visible within the disk. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a major merger or strong tidal interactions.
