The galaxy exhibits a distinct disk-like morphology, viewed nearly edge-on. There is a clear central bulge, appearing relatively smooth and concentrated. The disk appears moderately thick with some evidence of internal structure or dust lanes obscuring portions of the starlight. The galaxy's overall color appears relatively red, suggesting a population dominated by older stars, and possibly indicating a lower rate of on-going star formation within the galaxy. The shape is elongated, consistent with a disk galaxy observed at a high inclination angle. There is no obvious evidence of major mergers or significant tidal disturbances in the immediate vicinity of the galaxy, though minor perturbations or interactions cannot be ruled out.
