The galaxy presents as a dual-core system, suggesting either a binary galaxy or a major merger in progress. Each core exhibits a concentrated, smooth morphology, with a significant fraction of the overall light emitted from these central regions. Faint extensions of light can be seen around each core. Overall shape appears somewhat elongated. The color is generally yellow to white, indicating a population of older stars and a lack of significant ongoing star formation. There may be some signs of disturbance between the two cores, likely due to gravitational interactions.
