The galaxy appears as a flattened, elliptical structure. It presents a smooth, diffuse light profile with no discernible spiral arms or significant dust lanes. Its overall shape is elongated, approximately cigar-shaped, suggesting a classification between a spherical and a highly flattened elliptical galaxy. The light distribution suggests a relatively homogenous stellar population, without clumpy regions of star formation. There is a subtle color gradient across the galaxy, with a slightly bluer hue in the central region that fades to a redder hue in the outer edges. This color gradient indicates a possible variation in stellar populations or dust content across the galaxy. The galaxy shows no signs of tidal disturbances or interactions with other galaxies.
