The galaxy appears to be a spiral galaxy viewed edge-on. There is a central bulge that is slightly brighter than the rest of the disk. The disk appears relatively smooth with little to no visible structure such as spiral arms or dust lanes. Its light is skewed slightly toward the redder end of the spectrum. The lack of distinct features suggests a relatively quiescent star formation rate. There is no evidence of any major merger events, nor is there significant disturbance in the galaxy's structure, suggesting it has been relatively isolated for a considerable period of time. The galaxy appears to be elongated along its major axis, consistent with an edge-on orientation.
