The galaxy presents as an elongated, cigar-shaped structure. A prominent central bulge exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the center, the galaxy fades into a bluer, less defined disk. The disk appears relatively smooth, with no apparent spiral arm structure or significant dust lane obscuration visible in this image. There is no obvious sign of any major mergers or tidal disruptions in this image, with only a slight hint of a potential minor disturbance. Overall, the galaxy appears as a relatively quiescent system.
