The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a somewhat elliptical morphology, appearing more elongated than perfectly circular, but not cigar-shaped. The central region displays a yellowish hue, suggesting an older stellar population. Moving outward from the core, the color transitions towards a slightly bluer shade. The outer regions lack distinct spiral arm structures and show a smoother, more diffuse distribution of light, with faint hints of disturbance. There is no obvious central bar, and the galaxy shows no signs of major merger activity, although minor disturbances cannot be ruled out. Overall, it has a notable luminosity, and exhibits an appreciable rate of star formation.
