The galaxy appears to be a luminous elliptical, characterized by a smooth, relatively featureless morphology. Its color profile suggests a concentration of older stellar populations, with a dominant yellow-orange hue. There is no visible spiral structure or prominent dust lanes. The galaxy exhibits a high degree of radial symmetry, appearing almost perfectly round. There are no signs of ongoing mergers or major tidal disturbances, although it is difficult to completely rule out minor interactions. The central region of the galaxy exhibits a higher surface brightness, indicative of a dense stellar population in the core. Overall, the galaxy appears to be a well-formed, evolved system.
