The galaxy presents as an elliptical morphology, with a high degree of central concentration. It appears relatively smooth, lacking prominent spiral arms or distinct features indicative of active star formation regions. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central region. The galaxy exhibits a slight elongation, though it is predominantly round in appearance. There are no visible signs of ongoing mergers or major disturbances within the galactic structure, although subtle irregularities in the outer regions cannot be ruled out without higher resolution imaging. The light profile appears consistent and symmetrical, further supporting the classification as a relaxed, early-type galaxy.
