The galaxy presents as a diffuse, somewhat amorphous, aggregation of light. It has a non-distinct central condensation, with an irregular shape, lacking obvious spiral arms or a well-defined elliptical structure. The color profile shows a mix of hues, with regions of enhanced reddish tones, particularly in the central area, indicative of potentially older stellar populations or dust obscuration. There are hints of bluer regions scattered within the galaxy's broader emission, perhaps suggesting pockets of recent star formation. There are distortions in the shape of the galaxy that possibly indicate a current or recent merger. Light output is significant, inferring a reasonably large and luminous system. The galaxy appears actively merging, with a tidal tail or some sort of distortion.
