The galaxy presents as a centrally concentrated, luminous object with a smooth, elliptical morphology. The light is dominated by a yellowish-orange hue, suggesting a population of older stars. There is little evidence of spiral arms or distinct features, lending credence to its smooth and rounded appearance. The lack of discernible dust lanes or knots indicates a relatively low rate of current star formation. A faint, diffuse halo or extended envelope surrounds the central region, though the boundaries are indistinct and appear to fade gradually into the background sky. The overall symmetry suggests a dynamically relaxed system.
