The object presents as a single, relatively compact galaxy. It exhibits a generally smooth morphology with a near-circular profile, showing little indication of a disk structure or spiral arms within the resolution afforded by this image. The primary concentration of light is located at the center, implying a significant central bulge or nucleus, with a gradual decrease in luminosity outwards. There is no definitive evidence of ongoing merger activity or strong tidal distortions, and the system appears largely undisturbed. Faint extensions or halos may be present. The color suggests it is dominated by an older stellar population, but its actual redshift and intrinsic luminosity would be needed for further analysis. 