The galaxy presents a generally smooth and elliptical morphology, appearing somewhat elongated along a discernible axis. The central region exhibits a high degree of luminosity, suggesting a concentrated stellar population or possibly an active galactic nucleus. The galaxy displays a color gradient, with the core appearing more yellow/red, indicative of an older stellar population, while the outer regions transition to a slightly bluer hue, which may suggest the presence of younger stars or ongoing, though subdued, star formation. There are no prominent spiral arms or distinct dust lanes visible in this image, and it appears relatively undisturbed, showing no strong signs of recent or ongoing major mergers, although there is some visual suggestion of a very mild asymmetry or minor disturbance on one edge of the galaxy. The object is relatively compact.
