The galaxy presents a disturbed morphology, with a primary, somewhat spheroidal component and an apparent tidal tail extending outwards. The central region exhibits a concentrated, bright core, suggesting a high density of stars and possibly an active galactic nucleus. Colors appear bluer in the tidal tail, which could signify recent star formation activity. The galaxy displays an overall redder hue in the core. The overall shape appears to be irregular. The galaxy is likely undergoing or has recently undergone a merger event.
