The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. Its shape is close to circular, with only a slight elongation, appearing nearly face-on. The central region is bright and yellowish, suggesting a population of older stars. Fainter blue hues are visible in the outer regions, which might indicate the presence of some younger stellar populations or ongoing, albeit low, star formation. No distinct spiral arms or bar structures are discernible. The galaxy appears relatively undisturbed with no prominent signs of any major merger events.
