The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a dominant, smooth bulge that is approximately symmetrical. The central region of the galaxy is yellowish-white, suggesting an older stellar population. A faint, bluish disk component is observed, implying the presence of some younger stars and possible ongoing, albeit low-level, star formation. There is a notable lack of prominent spiral arm structures, leading to the classification of smooth featured. The galaxy has a slight elongation that can be described as in between round and cigar shaped. Furthermore, there is a minor disturbance detected, suggesting a possible interaction with a smaller companion or a past minor merger event.
