The galaxy exhibits a disturbed morphology, potentially indicative of an ongoing or recent merger event. The primary body of the galaxy appears elongated with a brighter, more condensed region transitioning to a fainter tail-like structure. The color gradient shifts from bluer hues in what may be an actively star-forming region, to yellower/redder tones in other parts of the galaxy, possibly indicating areas of older stellar populations. A significant fraction of the light appears concentrated, though there is a clear deviation from a perfectly elliptical or smooth profile. Evidence suggests the presence of some tidal features or asymmetries. A high probability of merger activity is noted due to the disrupted shape and irregular light distribution.
