This galaxy presents a disturbed morphology, suggestive of a possible ongoing or recent interaction. The central region exhibits a brighter, concentrated core with what appears to be a disk. There is a definite tidal tail or arm visible extending from one side of the main body, lending weight to the interaction hypothesis. There appears to be evidence of recent star formation. The redness on the edges suggests regions of dust obscuration. The estimated size indicates this is a moderately sized galaxy. Overall, a complex structure indicative of a dynamic system.
