The galaxy presents as an elliptical morphology with a smooth, concentrated light profile. The central region exhibits a brighter, more intense yellowish-orange hue, suggesting a population of older stars. The outer regions transition to a greenish hue, which may indicate the presence of some younger stars or ionized gas, although this is not very prominent. The galaxy displays a slight elongation, appearing more like a flattened spheroid than a perfect sphere. There is no noticeable spiral structure or any signs of significant tidal disturbances or ongoing mergers in the immediate vicinity based on the morphology; the galaxy is a relatively isolated system. The overall structure suggests a galaxy that has largely completed its star formation, though some low-level activity is still likely occurring.
