The galaxy presents as a relatively compact object with a smooth overall appearance. The central region exhibits a prominent, concentrated bulge that appears largely spheroidal. There is a notable color gradient, with the bulge displaying a more yellow/orange hue, suggestive of an older stellar population or significant dust extinction. Fainter disc is present around the central bulge.

There is evidence that there is a possible interaction or disturbance, given that the merging fraction is nearly one-third.