The galaxy presents as a lenticular or possibly a spiral galaxy viewed nearly edge-on from our perspective. It appears elongated with a bright central bulge and a relatively faint disk component. There is a slight warping in the disk structure suggestive of possible past interactions. The dust lane obscuring the central bulge appears as a thin, dark band running across the major axis. Star formation activity appears to be low, with no prominent star-forming regions visible in this band.
