The galaxy presents as a somewhat diffuse object, exhibiting a generally elliptical morphology. The central region appears significantly brighter and concentrated, suggesting a prominent bulge. Fainter, extended emission surrounds the core, though the outer edges lack sharp definition, potentially indicative of a low surface brightness disk or halo. There is a slight color gradient, with the core displaying a yellow-orange hue, possibly indicative of an older stellar population, while the outer regions may be slightly bluer. Overall, the galaxy appears to be undergoing or have undergone a merging process with another galaxy.
