The galaxy appears to exhibit a complex morphology, possibly indicative of an ongoing or recent merger event. There are two dominant, rounded, yellowish components. A fainter, bluish component is visible in close proximity to the brighter yellowish components, suggesting a possible tidal tail or star-forming region triggered by the gravitational interaction. The overall shape deviates from a regular elliptical or spiral structure. A distinct amount of disturbance is visible in the structure of the galaxy. The light distribution across the object is not uniform. There is evidence of possible star formation occurring within the system, indicated by bluer regions, though the bulk of the stellar population appears older, given the prevalence of yellow/red hues in the brighter components.
