The galaxy presents as a relatively smooth, centrally concentrated object, likely an early-type galaxy given its lack of prominent spiral arms or disk-like structure. The core region exhibits a yellowish-orange hue, suggesting an older stellar population. A subtle greenish-blue tint is observed in the outer regions, possibly indicating the presence of younger stars, or ionized gas. The galaxy appears slightly elongated. No obvious signs of ongoing major mergers or tidal disturbances are detected. The galaxy is not perfectly spherical; it leans towards an elliptical shape.
