The galaxy presents a generally smooth and concentrated appearance. It appears largely elliptical, with a notable central bulge. The light profile shows a high degree of central concentration, diminishing in intensity towards the outer regions.  There is a distinct lack of discernible spiral arm structure. The galaxy exhibits a color gradient, appearing yellower and redder in the central regions, suggesting a population of older stars with lower metallicities, which could potentially indicate a small degree of past or current star formation. There are no obvious signs of active galactic nuclei activity or major disturbances from interactions with other galaxies.  The galaxy does not appear particularly flattened. Its overall symmetry suggests it is a relatively relaxed system.
