The galaxy presents a generally elliptical morphology, though not perfectly spherical, showing a slight elongation. Its overall structure is smooth, with no readily apparent spiral arms or distinct features. The color gradient suggests a higher concentration of older stellar populations, particularly in the central bulge, which appears brighter and slightly redder. The outer regions of the galaxy exhibit a more subtle blue hue, indicative of some ongoing, albeit subdued, star formation. No significant tidal disturbances or interactions with other galaxies are immediately visible.
