The galaxy presents as a system with a complex morphology, potentially indicative of an ongoing or recent merger event. Two distinct nuclei are observed. The primary nucleus exhibits a smooth, elliptical-like structure. A secondary, somewhat smaller nucleus is located nearby; it possesses a more irregular, disturbed appearance. The system shows a generally circular shape but significant distortions are apparent, potentially attributed to tidal interactions. The overall color profile suggests a significant population of older stars. Evidence of star formation might be subtle, but can't be ruled out given the disturbed morphology.
