The galaxy presents as a system undergoing a merger. Two distinct galactic nuclei are visible, both exhibiting a yellowish-orange hue suggestive of an older stellar population. The morphology appears significantly disturbed, with a noticeable lack of defined spiral arms or a smooth elliptical structure, indicating strong gravitational interactions. A faint, diffuse envelope of stellar material surrounds both nuclei, implying tidal stripping and the ongoing exchange of matter between the merging components. The overall luminosity suggests a relatively massive system. Star formation appears to be suppressed or occurring at a low rate, consistent with the observed color and the advanced stage of the merger. Dust lanes, if present, are not clearly discernible within the available image resolution. Evidence of strong tidal tails or prominent merger remnants are suggested.
