The galaxy presents as a centrally concentrated, flattened ellipsoid. Its color suggests an older stellar population, with a predominantly red-yellow hue dominating the central region. The galaxy appears smooth in texture, lacking any prominent spiral arm structures or significant dust lanes. The light profile suggests a gradual decrease in luminosity from the center outwards, indicating a lack of recent major star-forming events. The galaxy's elongated shape suggests it could be either an elliptical galaxy with intrinsic flattening or a disk galaxy viewed at a high inclination. There is no visible evidence of a recent major merger or significant tidal disturbance. Faint, diffuse extensions or a halo might be present but are indistinct.
