The galaxy exhibits a complex morphology, characterized by features indicative of an ongoing or recent interaction or merger. The overall form is asymmetrical, showing a departure from a simple elliptical or spiral structure. The central region appears relatively smooth. One prominent feature is a disturbed arm that extends outwards. Bright knots of star formation are suggested. The galaxy's color suggests the presence of an older stellar population mixed with pockets of recent star formation. There is evidence of tidal tails and disrupted structures, further indicating gravitational interaction. The overall impression is that of a dynamically active system.
