The galaxy presents as a moderately luminous object with a smooth, centrally concentrated morphology. It exhibits a slight elongation, appearing somewhere between round and cigar-shaped. The primary structure displays a gradient in color, with a region of bluer light visible to one side of its core, that may suggest a zone of active star formation. The bulk of the light appears to come from older stars, and the redder color to the opposing side may suggest a difference in stellar population age, or high amounts of dust obscuring the region. There is visual evidence of an interacting galaxy, or tidal debris to the right of the main body, suggesting a previous or ongoing gravitational interaction. The overall structure does not indicate any significant features such as spiral arms or a distinct disk, but rather a more spheroidal shape.
