The galaxy presents as a disrupted system, potentially in the late stages of a merger event. Morphologically, it exhibits characteristics of both a smooth, elliptical-like structure and a disturbed disk. A bright, somewhat spherical central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population. Emanating from one side of the bulge is faint wispy structure, hinting at tidal tails and disruption of a disk.

To the right of the bulge is a second somewhat concentrated area, with the barest hints of structure. This may be a disrupted component of the merger. The overall color of the galaxy suggests a significant population of older stars, though hints of blue suggest some ongoing, albeit low-level, star formation may be present. The general morphology suggests a massive galaxy that has undergone or is undergoing significant gravitational interaction.
