The galaxy presents as a somewhat diffuse, centrally concentrated object. It displays a primarily smooth morphology, with an overall yellowish-red hue suggesting an older stellar population, although some bluer emissions are visible. The shape is neither perfectly spherical nor elongated. A notable characteristic of this galaxy is the existence of what appears to be a dual core, which could be a secondary distinct nucleus. Alternatively, this could be a case of galactic merging or tidal interactions. Further spectroscopic and higher resolution imaging is needed to confirm these hypotheses and determine the dynamics of the object.
