The object appears to be a spiral galaxy, viewed almost entirely edge-on from our line of sight. There is a clear, thin disk structure evident, with obscuring dust lanes visible against the brighter galactic bulge. The central bulge is prominent, and appears to be mostly spheroidal with a slightly oblong shape. It exhibits a smooth texture with light concentrated towards the center. The disk is composed of older stars, and there are no clear arms. There is no evidence of any interactions or signs of a major merger. The galaxy does not display strong irregularities in shape or a diffuse halo.
