The galaxy presents an elongated, disk-like morphology, suggestive of a spiral or lenticular galaxy viewed at a high inclination angle. There is a central bulge with a more concentrated and smooth light distribution. Fainter, diffuse spiral arm structures are suspected but not clearly defined, hinting at ongoing, albeit potentially weak, star formation. The overall color of the galaxy appears bluish, indicative of a relatively young stellar population, though this is subtle. No clear signs of major mergers or tidal disturbances are observed. The galaxy exhibits a relatively smooth texture.
