This galaxy exhibits a generally smooth morphology, appearing largely featureless in this image. It appears to be undergoing a merger or interaction with another galaxy, as evidenced by the twin-nuclei or disturbed structure, suggesting a non-relaxed system. The primary light emission is concentrated in the central region, which appears relatively round. The color profile is generally yellowish, indicating a population of older stars, with relatively low ongoing star formation. The overall appearance suggests an evolved system undergoing a significant gravitational interaction.
