The galaxy presents as a largely smooth, elliptical-like structure. It is generally round in appearance, with a slight central concentration of light. The core exhibits a somewhat pinkish hue, which could indicate ongoing or recent star formation within the galaxy's center. The outer regions of the galaxy show a blueish tint, though subtle, which suggests the presence of a younger stellar population relative to the core. There is no evidence of distinct spiral arms or a prominent disk-like structure; the overall light distribution appears fairly uniform and diffuse. There are no signs of any major disturbances or tidal features suggesting recent mergers. Overall, the galaxy looks like a relatively quiescent system.
