The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The core region displays a bright, yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy show a gradual decline in luminosity and a bluer tint, possibly indicating the presence of younger stars or a lower metallicity. There is no evidence of spiral arms or a prominent disk structure. Subtle irregularities and a slight extension can be seen on one side, which could indicate minor gravitational disturbance, perhaps caused by a past interaction or ongoing accretion. The galaxy is generally round in appearance, with only a slight deviation from perfect circularity. Overall, the galaxy presents the appearance of a massive, relatively quiescent system with little active star formation.
