The galaxy presents a somewhat elliptical morphology with a noticeable bulge region. A disk component is present, with an inclination that suggests it is close to face-on. The bulge exhibits a smoother texture and a yellowish hue, suggesting an older stellar population. The disk appears less structured, showing a mottled texture which could be due to dust obscuration. Overall, the galaxy appears relatively undisturbed, without any obvious signs of ongoing major mergers or tidal interactions.
