The galaxy presents a complex morphology. The primary body appears relatively smooth and elliptical in shape. A fainter region exhibits a more irregular structure. The elliptical component presents a primarily yellow-orange hue, suggestive of an older stellar population. A region of bluish light is also present, concentrated in what appears to be irregular structures. These bluish components suggest the presence of younger, hotter stars and active star formation. The light concentration is not uniform, but rather appears clumpy. Overall, the galaxy displays evidence of possible tidal features, which might indicate interaction or a minor merger.
