The galaxy presents an elliptical morphology, appearing largely smooth and concentrated towards the center. The light distribution is centrally-peaked with a gradual decrease in luminosity outward from the core. There is a slight elongation, deviating from a perfectly circular shape. There is no apparent structure such as spiral arms or a distinct disk component. Color gradients suggest the central region exhibits a yellower hue, indicative of an older stellar population, while the outer regions appear slightly bluer. Based on the overall color profile and morphology, this galaxy is likely a massive system that is not actively forming many stars. There may be signs of a past minor disturbance, but nothing significant.
