The galaxy presents as a somewhat diffuse, centrally concentrated object. It appears largely smooth in texture, lacking well-defined spiral arms or a prominent bar structure. The core region exhibits a yellowish hue, possibly indicating an older stellar population or dust obscuration. Moving outward from the core, a subtle blueish tint is observed, potentially suggestive of younger stars. The overall shape is nearly circular. There is no obvious evidence of strong tidal interactions or recent major mergers, though some minor irregularities in the outer regions cannot be ruled out. The galaxy's color indices suggest ongoing star formation at a moderate rate.