The galaxy presents as a relatively smooth, disk-shaped object with a centrally concentrated bulge. The light distribution is notably more concentrated toward the center, suggesting a higher stellar density in the core region. The galaxy exhibits a slight elongation, with an apparent axis ratio suggesting a mildly inclined disk. Faint, diffuse emission extends outwards from the central region, fading into the background. Color gradients are subtle, with a slightly bluer hue in the outer regions compared to the more yellow-red central bulge, potentially indicating ongoing star formation in the disk. There are no obvious signs of strong spiral arm structure or major disturbances, implying a relatively undisturbed morphology.
