This galaxy presents a complex morphology, suggestive of an ongoing or recent interaction. The primary component exhibits a generally smooth light distribution, however there appears to be distortions in the form of what seems to be tidal tails. There appears to be a second object, close in proximity. A fraction of the galaxy appears slightly bluer in color compared to other portions of the galaxy. This may be indicative of younger stellar populations or ongoing star formation. The overall structure is somewhat diffuse, suggesting a less centrally concentrated mass distribution. The color profile indicates a likely intermediate-redshift object. The galaxy is not perfectly spherical and appears slightly elliptical. Some features are indicative of the galaxy undergoing a merger, although some of the features could be considered minor disturbances.
