The galaxy exhibits a relatively smooth morphology, appearing largely featureless across the observable spectrum. It presents a highly circular shape, showing minimal deviation from a perfect circle. There is little to no discernible structure suggesting spiral arms or a distinct galactic disk. The galaxy's color profile indicates it emits strongly in the green band, but there is limited to no emission in the redder bands. This could indicate the presence of a unique chemical composition. There is no obvious evidence of ongoing or recent major merger activity, though subtle signs of minor disturbances cannot be completely ruled out. The overall light distribution is concentrated towards the center, gradually diminishing in intensity towards the edges, which suggests a high degree of symmetry and potentially an older stellar population. The core of the galaxy appears to be more condensed than the outer halo.
