The galaxy presents a generally smooth, rounded morphology. There's a central, highly luminous region, likely indicative of a concentrated galactic nucleus. Fainter diffuse light extends outwards from the core, fading gradually into the background. There is a hint of some structural irregularity or disturbance in the extended halo. While generally smooth, there are also traces that potentially suggest ongoing or recent merging activity which may contribute to its luminosity and star formation rate. Overall, the galaxy appears relatively featureless, with no clear indication of spiral arms or a well-defined disk structure from the image, though some asymmetry seems to be present in the halo around the core.
