The galaxy exhibits a morphology suggesting an ongoing or recent merger event. Its overall structure appears disturbed, with evidence of tidal features or extended arms. The central region displays a concentrated luminosity, potentially indicating an active galactic nucleus or a dense stellar population. The galaxy's color profile suggests a mix of stellar populations, with some regions appearing bluer, possibly indicative of active star formation, and others redder, suggesting older stellar populations. The general shape is elongated but is transitioning from smooth to having more distinct features. There appears to be at least one major disturbance, and a likely merger.
