The galaxy appears as a single, somewhat asymmetrical object, likely an elliptical galaxy based on its smooth, featureless morphology. There is an area of relatively high surface brightness concentrated near the center, exhibiting a yellowish hue, suggestive of an older stellar population. The outer regions of the galaxy exhibit a diffuse, indistinct boundary, indicating a gradual decline in stellar density with increasing radius. A slight elongation is visible in the structure, though the axial ratio appears to be relatively high, implying a nearly circular shape.

There are two distinct components. The brighter of the two has a distinct smooth profile, with little structure and a high concentration of light near the core. The dimmer component appears to be more diffuse, with a slight disk-like shape. Faint, elongated color variations are visible in this component.
