The galaxy appears to be a spiral galaxy viewed at a moderate inclination. It exhibits a bright, relatively smooth central bulge, with a yellowish-white hue suggesting an older stellar population. The disk component displays a more mottled texture, with hints of spiral arm structure emerging from the central bulge, these arms contain regions of bluer light, which are probably areas of active star formation. The overall color profile indicates a mix of stellar ages throughout the galaxy. Some minor asymmetry is visible in the disk, this could be a tidal disturbance from a small interaction but may also be internal to the structure of the galaxy. The general morphology suggests that this galaxy is an intermediate spiral, not strongly barred, and not heavily structured. 
