The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a bright, yellow-white hue. The surrounding halo demonstrates a gradual decrease in luminosity and a shift in color toward a bluer, though still relatively subdued, tone. There are faint indications of a slight disk-like structure, but this feature is not well-defined. No significant tidal features or distortions are apparent, suggesting the galaxy is not currently undergoing a major merger event. The galaxy appears relatively isolated, showing no clear signs of interaction with nearby galaxies. There is evidence of ongoing star formation, though at a low rate, indicated by the slight blue color in the outer regions. Overall, the galaxy appears to be a mature, relatively quiescent system.
