The galaxy presents as a largely featureless elliptical morphology. It exhibits a centrally concentrated bulge that appears yellow-white in color, suggesting an older stellar population. The radial color gradient indicates a slight bluer hue in the outer regions relative to the core, possibly indicating a younger or more metal-poor stellar population compared to the core. There is no evident dust lane or spiral structure, and the overall appearance is smooth and spheroidal, with a very slight elongation. There is no apparent evidence of an active galactic nucleus. The galaxy is relatively compact.
