The galaxy appears to be a luminous, elliptical morphology, exhibiting a centrally concentrated light profile. The core region is bright and diffuse, suggesting a high stellar density. The isophotes appear relatively smooth, indicating a well-mixed stellar population. There is a slight flattening of the galaxy's shape, deviating somewhat from a perfect circle, possibly due to rotation or tidal interactions in its past. Color gradients are subtle, with a tendency towards redder hues in the central bulge and slightly bluer tones in the outer regions. The overall color profile indicates an older stellar population, potentially implying a low rate of current star formation. No distinct spiral arms or dust lanes are visible, further supporting its classification as an elliptical galaxy.
