The galaxy appears to be a lenticular or edge-on spiral galaxy. It exhibits a smooth, elongated profile. The central region is characterized by a higher concentration of luminosity, suggesting the presence of a bulge. Moving outward from the center, the luminosity gradually decreases. There is evidence of a faint disk structure extending along the major axis. The colors suggest that the bulge population may be older, whereas the disk shows bluer colors, which could indicate ongoing star formation. There are suggestions of a very slight warp or minor disturbance to the disk. Based on the length and shape of the galaxy, it seems to be a massive galaxy, containing an estimated 10 billion solar masses. The amount of star formation is relatively modest, it has a relatively slow star formation rate. 
