The galaxy presents as a relatively smooth, elongated structure. The overall shape is cigar-like, with a high degree of axial ratio. The central bulge appears to be a yellow-orange color, suggesting an older stellar population. Moving outward from the center, the galaxy fades into blue hues, possibly indicating the presence of younger stars in the outer regions. There is a subtle asymmetry visible in the distribution of light, with a slight extension or disturbance on one side. The galaxy lacks a pronounced spiral structure or any obvious signs of active star formation on a large scale.
