The galaxy presents as an interacting system, potentially in the late stages of a merger. There appear to be two distinct nuclei visible, one with a more diffuse, ring-like structure surrounding it. The central regions of both nuclei show a concentrated luminosity, suggestive of older stellar populations. The ring around one nucleus may be a tidal feature resulting from the gravitational interaction. A faint bridge of material seems to connect the two nuclei, which suggests gravitational interaction. Overall, the system exhibits an irregular morphology. A lack of strong blue light suggests relatively low levels of current star formation activity within the observable regions. The galaxy is neither perfectly elliptical nor a clear spiral, exhibiting a complex, perturbed structure. The overall luminosity suggests a galaxy with a substantial stellar mass.
