The galaxy presents as a centrally concentrated, smooth elliptical morphology with a slight elongation. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. The galaxy's color profile transitions towards a redder hue as it extends outwards from the core, indicating a potential decline in ongoing star formation further from the center. No prominent spiral arms or disk-like structures are apparent. Minor disturbances are suspected due to the asymmetry of the galaxy shape. The general roundness suggests a relaxed system approaching equilibrium.
