The galaxy presents as an elliptical morphology, appearing largely smooth and rounded. The color profile indicates a concentration of older stellar populations, with a yellowish hue dominating the central bulge region. The light is fairly concentrated within the center, hinting at a relatively high mass. There is little evidence of active star formation, suggested by the lack of distinct blue or irregular features typically associated with younger stars and star-forming regions. The overall structure does not obviously suggest any recent major merger activity, although a slight asymmetry might indicate a minor interaction in the galaxy's past.
