The galaxy presents as a somewhat diffuse, centrally concentrated object. The overall color appears bluish, suggesting the presence of a moderate population of younger, hotter stars. The morphology is difficult to classify precisely given the resolution of the image, but it appears largely smooth and elliptical, with a slight elongation. There are no obvious spiral arm structures or prominent dust lanes visible. It is likely a galaxy with a substantial stellar mass and moderate levels of star formation. There is some indication of minor disturbances or interactions, although the galaxy appears generally isolated.
