The galaxy presents a somewhat amorphous structure, exhibiting an overall elliptical shape. A central, brighter region is visible, potentially indicating a nucleus or a denser concentration of stars. Diffuse spiral arm structures appear to emanate from this central region, though they lack sharp definition. The galaxy displays a bluer hue, which might suggest ongoing or recent star formation. There appear to be some structural irregularities in the overall form, possibly indications of an interaction or merger event. The surface brightness of the galaxy appears to fade gradually from the core to its outer edges.
