The galaxy presents a generally smooth and rounded morphology. A central, bright, and slightly concentrated bulge is evident. The outer regions exhibit a gradual fading in luminosity, suggesting a diffuse stellar halo or envelope. There are no readily apparent spiral arms or bar structures, which indicates that it is an elliptical galaxy with a large quantity of older stars with low star forming capabilities. There are some subtle color variations in the outer regions, appearing as faint patches or irregular shapes, suggesting either tidal disturbances or active galactic nuclei.
