This galaxy exhibits a primarily smooth morphology. The central region displays a bright, concentrated core that graduates outward into a more diffuse halo. The general shape appears elliptical, tending toward roundness but noticeably flattened. The color profile indicates an older stellar population. The inner core shows yellowish-white coloration with a green band at the bottom, suggesting possible intermediate-age stars or ongoing, albeit minimal, star formation. The outer regions exhibit a redder hue consistent with an aging stellar population. No prominent spiral arms, dust lanes, or tidal features are observed. The galaxy appears relatively undisturbed, with no signs of major mergers or interactions. Overall, this galaxy can be described as an elliptical galaxy with minimal star formation and an aging stellar population.
