The galaxy presents as a luminous, elliptical-shaped object. Its morphology appears largely smooth and featureless, with a concentrated central bulge and a more diffuse halo. The light profile suggests minimal disk-like structure. 

Coloration is predominantly in the redder wavelengths, indicating a population of older stars and a low rate of ongoing star formation. The object displays an overall roundness, lacking the elongated or cigar-like appearance that might suggest a more active or disturbed system. There is no obvious evidence of major mergers or tidal disturbances in this image, though subtle asymmetries might indicate minor past interactions.
