This galaxy presents a complex morphology, exhibiting features suggestive of an ongoing or recent merger event. The primary body of the galaxy appears somewhat amorphous, lacking a clearly defined spiral or elliptical structure. There is a notable tidal tail extending outward from the central region, indicating gravitational interaction and disruption. The color distribution within the galaxy is uneven, with a concentration of bluer hues in some areas, possibly indicative of younger stellar populations or active star formation. A smoother, more yellow/red hue is also present. The presence of these features suggests the galaxy is not in a state of equilibrium and has likely experienced significant dynamic processes.
