The galaxy presents as a single, concentrated object with a centrally dominant, bright core. The morphology is generally smooth and elliptical in appearance, with a noticeable lack of defined spiral arms or a prominent disk structure. The color profile shifts from yellow-white at the core to redder hues in the outer regions, suggesting an older stellar population predominating, with a low rate of ongoing star formation. There is little evidence of significant dust lanes or recent merger activity based on any clear morphological disturbances, though a slight distortion in the halo could indicate minor past interaction. The galaxy is likely a massive system. Its overall form points towards it being an evolved galaxy.
