The galaxy appears as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge and a gradual decrease in brightness towards its outer edges. It presents a yellowish-orange hue, suggesting an older stellar population, with minimal evidence of recent star formation. The isophotes are generally regular and concentric. The galaxy appears isolated, showing no signs of major interactions or mergers with other galaxies, and only very minimal distortion of the main body.
