The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a high concentration of light, appearing nearly circular and gradually fading outward. There is minimal evidence of distinct spiral arms or prominent dust lanes. The overall color profile is dominated by yellow and red hues, which indicates an older stellar population with lower rates of active star formation. It appears relatively undisturbed, with no signs of major mergers or significant tidal features. Faint extensions suggest subtle interactions or past minor mergers. The galaxy’s light profile suggests a predominantly bulge-dominated system.
