The galaxy presents a smooth, elliptical morphology. Its color profile indicates a dominance of older stellar populations, emitting light primarily in the redder regions of the spectrum. The galaxy's light distribution is concentrated towards the center, indicating a significant bulge component. There is a subtle asymmetry present, perhaps suggestive of a minor interaction or disturbance. Overall, the structure appears relatively relaxed, with no obvious signs of active star formation or strong tidal features. It would be reasonable to classify this galaxy as an early-type, potentially undergoing a merger event in the distant past.
