The galaxy appears as a relatively faint, elongated structure with a disk-like morphology viewed at a significant inclination. The central region shows a slightly brighter concentration of light, possibly indicating a bulge. The disk exhibits some patchy features and irregularities, suggesting ongoing star formation and/or dust obscuration. Faint tidal features or distortions are present, hinting at possible gravitational interactions or past mergers. Overall, the galaxy presents a moderately disturbed appearance, with the possibility of minor merger activity.
