The galaxy presents as a somewhat irregular, ellipsoidal structure. There is a concentrated, bright central region exhibiting a yellowish hue, suggestive of an older stellar population. The light distribution suggests that the galaxy is likely in transition from a spiral to elliptical. The estimated physical size indicates this is a typical size galaxy. It also appears that the galaxy is composed of two parts that are merging. The galaxy's overall shape deviates somewhat from a perfect ellipsoid.
