The galaxy appears to be a luminous, elliptical system, exhibiting a smooth and relatively featureless morphology. Its light profile suggests a centrally concentrated bulge, with a gradual decrease in luminosity extending outwards. There is little evidence of spiral arms or distinct disk structures. The galaxy displays a yellowish-orange hue, possibly indicative of an older stellar population and lower ongoing star formation activity. The system seems largely undisturbed, lacking prominent tidal features or signs of major mergers. A slight elongation is observed, suggesting it is not perfectly spherical. Overall, the galaxy presents characteristics consistent with a massive, evolved system with minimal current star formation.
