The galaxy appears to be relatively smooth in morphology, lacking prominent spiral arms or a distinct bar structure. There is a possible central bulge that is brighter than the surrounding disc. The galaxy has a generally rounded shape. The object does not obviously appear to be undergoing any major merging activity or strong tidal disturbances, though there might be a minor perturbation present. There appears to be some star formation occurring within the galaxy as indicated by the slight bluish tint. Overall, the galaxy appears to be an early-type spiral or possibly a lenticular galaxy.
