The galaxy appears to be a lenticular or early-type spiral galaxy seen edge-on or at a high inclination. It exhibits a notable central bulge that dominates its structure, appearing smooth and concentrated with a yellowish hue, suggesting an older stellar population. The disk component is less pronounced, but is more cigar shaped than circular. Evidence of dust lanes or spiral arms is not readily apparent, indicating a lack of significant ongoing star formation.

A smaller, fainter, and more diffuse object is located nearby that is either a satellite galaxy or a background object gravitationally lensed by the target galaxy. The apparent smoothness and lack of distinct features in the primary galaxy suggests it is relatively evolved and likely contains a substantial stellar mass. The very low estimated specific star formation rate supports that the galaxy is relatively quiescent and not actively forming many new stars.
