The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated, spheroidal shape with a high degree of central light concentration. The light distribution suggests an absence of prominent spiral arms or disk-like features. The galaxy appears to be relatively isolated, without any obvious signs of major tidal disturbances or ongoing mergers with other galaxies. Its color gradient indicates a population of older stars, with the core emitting a yellowish-orange hue. The outer regions of the galaxy appear dimmer, suggesting a gradual decline in stellar density. Overall, the galaxy appears to be a quiescent, early-type system.
