This galaxy presents an elongated, disk-like morphology, viewed at a significant inclination. There is evidence of a bulge, a central concentration of light that appears more yellow. Fainter and bluer light emanates from the outer regions, indicating the presence of a stellar disk. Irregular features are observed that may indicate some signs of disturbance. Overall, the galaxy does not present a completely smooth appearance, exhibiting some amount of substructure. It is likely a spiral galaxy viewed at an oblique angle, but the spiral arms are either faint, tightly wound, or disrupted.