The galaxy presents a morphology consistent with a disk galaxy seen at an oblique angle, exhibiting a central bulge and a flattened disk. The bulge appears to be a dominant feature, characterized by a smooth, concentrated distribution of light, suggesting an older stellar population. The disk component shows some indication of structure, though not distinctly resolved into spiral arms. The overall color of the galaxy is yellowish-red, which, taken together with its morphology, may suggest an intermediate type, possibly undergoing some process of transformation, transitioning between being actively star-forming and quiescent. There is a faint disturbance in the disk, which may indicate a minor interaction. The galaxy is estimated to be a moderate-sized system with high mass and low star formation.