The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth, diffuse morphology. The light profile suggests a centrally bright bulge that fades gradually outwards. Color gradients indicate a yellowish hue in the central regions. There is little evidence of spiral arms or significant dust lanes. The overall symmetry of the light distribution suggests a relaxed system, potentially an early-type galaxy or a spiral galaxy viewed nearly face-on but where the arms are not distinct. There is no strong visual evidence of ongoing major mergers or tidal disturbances. The galaxy exhibits a slightly elongated shape. 
