The galaxy presents as a moderately bright, elliptical or lenticular-shaped object. The central region exhibits a concentrated luminosity gradient, appearing more intensely illuminated than the outer regions. The overall color profile leans toward the redder end of the spectrum, with a pronounced yellowish-orange hue dominating the core. The light from the galaxy diminishes gradually outward from the center, indicating a smooth transition to the surrounding background. There is minimal indication of spiral arm structures. The light distribution suggests the presence of an older stellar population. The object seems generally undisturbed, with a regular and symmetrical structure. There may be some subtle asymmetry in the outer edges, but further evaluation is necessary to determine if that is due to tidal disturbances.
