The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light distribution suggests a relatively featureless spheroidal shape, showing a transition between elliptical and disk-like. The roundness of the galaxy is between round and somewhat elongated. There is no clear presence of spiral arms or a bar structure. Evident is a distinct merging occuring with another object. There appears to be a primary galaxy with signs of tidal disruption or interaction visible in the image. The red color in the central regions indicate the presence of older stellar populations, implying relatively low current star formation activity. The overall color is slightly more concentrated in the longer wavelengths.
