The galaxy presents as a moderately inclined, disk-shaped structure. It exhibits a generally smooth appearance, with a concentrated central bulge region showing a yellowish-white hue. Moving outward from the core, the disk displays a bluer tint, suggesting the presence of younger stellar populations and ongoing star formation. The galaxy is relatively undisturbed, showing no strong signs of recent major merger events. The disk appears somewhat asymmetrical, possibly due to minor gravitational interactions or internal processes influencing the distribution of its stellar components. The light distribution gradually fades from the center to the outer edges.