The galaxy presents as a centrally concentrated, generally smooth structure. It exhibits a roughly circular morphology. The core region appears bright and relatively featureless. Proceeding outwards from the core, a gradual decrease in surface brightness is observed. The central region displays a yellowish hue, possibly indicating an older stellar population, with bluer tones in the outer regions. Overall, the galaxy appears to have a spheroidal shape with only minor deviations. There appears to be no clear evidence of spiral arms or a distinct disk structure.
