The galaxy appears to be a disk galaxy, viewed at a high inclination angle, appearing nearly edge-on. The central bulge region is prominent, exhibiting a brighter, more concentrated luminosity profile. The overall color is bluish-white, suggesting a stellar population of primarily intermediate to old stars with moderate star formation activity. The dust lane is not very prominent. Faint extensions or tidal features are not clearly evident, but some minor disturbances in the outer regions are present. The overall appearance suggests a relatively undisturbed galaxy that is not currently undergoing any major merger events.
