The galaxy presents as an edge-on spiral or lenticular type, exhibiting a prominent central bulge that appears relatively smooth and concentrated. The disk component is elongated, with a significantly greater length than width, indicative of a high inclination angle relative to our line of sight. Within the disk, there is some clumpy, asymmetric structure indicative of some minor disturbances. The color profile shows the central bulge as yellow-white, potentially indicating an older stellar population, while the disk exhibits bluer hues, suggesting more recent star formation. Overall the galaxy does not appear to have any major ongoing merger events, but there might be some tidal disturbance.
