The galaxy presents as a system with morphological disturbances. There appear to be at least two distinct galactic nuclei within a common envelope, possibly suggesting an ongoing or recent merger event. The primary nucleus appears elongated, with an irregular shape, and a yellowish hue, consistent with an older stellar population. A secondary, smaller and bluer component is adjacent to the first nucleus, indicating the possible presence of a region with younger, hotter stars. The overall form deviates significantly from a regular elliptical or spiral morphology, which suggests gravitational interaction. There are no obvious spiral arm structures.
