The galaxy presents with a relatively smooth morphology. The primary structure appears as a central bulge or core region exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. This core is somewhat elongated and appears to be undergoing significant gravitational interaction. Evident disruption is present near the main structure of the galaxy, and there is what looks to be a second smaller, bluish galactic structure. This may be due to a possible merger of galaxies.

The bluish coloration of the secondary galaxy suggests a population of younger, hotter stars, and the overall system gives evidence to substantial star formation. 
