The galaxy exhibits a complex morphology. It appears to be in a late stage merger. The main body is a relatively smooth, luminous spheroid with a yellowish hue. There is a smaller secondary component. The galaxy has an estimated diameter of around 11 kiloparsecs, making it a moderate-sized system. The overall shape is somewhat distorted from a perfect ellipse, indicating gravitational interaction. The light from the galaxy suggests a substantial population of older stars, though the color also indicates some ongoing, albeit low, star formation. There is the possibility of a tidal tail visible to the lower right of the galaxy. Further investigation is required to accurately classify its precise stage of evolution and to confirm the merging activity.
