The galaxy presents a generally smooth and somewhat featureless appearance, though subtle structures are discernable within its disk. The central bulge exhibits a concentrated, yellowish-white hue, indicative of an older stellar population. Moving outward from the core, the disk becomes more diffuse, with hints of spiral structure implied by slight variations in color and brightness. The overall color profile transitions from warmer tones in the center to slightly cooler hues towards the periphery. The disk is observed at a fairly high inclination, allowing for estimations of its radial extent. There is minimal evidence of major ongoing mergers or significant tidal distortions, although subtle asymmetry within the disk could suggest minor gravitational interactions or internal disturbances.&#x20;
