The galaxy appears to be a relatively smooth, elongated structure. It exhibits a distinct, cigar-like shape, with a brighter, more concentrated central region that fades into a diffuse outer disk. The color gradient suggests an older stellar population, with the central bulge appearing yellower, possibly indicating a higher concentration of evolved stars. There is a hint of a subtle disturbance on one edge of the galaxy. Overall, the galaxy seems to be a relatively undisturbed system.
