The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. There is a noticeable core, indicating a higher concentration of stellar mass or possibly the presence of an active galactic nucleus. The overall color of the galaxy appears relatively uniform, suggesting an older stellar population with little ongoing star formation. There are subtle indications of a possible slight disturbance in the morphology. The galaxy is generally round in appearance, without a distinct disk structure.