The galaxy presents as a single, relatively smooth object. The morphology is generally elliptical, appearing moderately elongated rather than perfectly spherical. A brighter, more concentrated central region is evident, suggesting the presence of a galactic bulge. Moving outwards from the center, the light gradually diminishes in intensity. Subtle color variations are observed, with a slightly bluer hue present in the outer regions, perhaps indicating ongoing star formation. There is no visually apparent structure such as spiral arms or a bar. There is no clear sign of interaction or significant disturbance in its shape, though the light may be slightly disturbed.
