The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, exhibiting a high degree of radial symmetry with little discernible disk structure. The light profile suggests a dominance of older stellar populations, indicated by the yellowish-red hue which dominates the galaxy's color. There may be some evidence of minor tidal disturbances or internal asymmetries in the light distribution. The bright central region suggests the presence of a dense stellar nucleus or potentially an active galactic nucleus, although the resolution does not allow for definitive confirmation.