The galaxy presents with a disk-like morphology, although some disturbances are present, perhaps suggesting a past minor merger event. The central bulge is moderately bright with an elliptical shape. Blue hues are visible in the disk, possibly indicating the presence of younger stars. There appears to be no prominent central bar structure within the disk. There are some minor disturbances within the disk itself. The overall color index indicates some degree of star formation is occurring. The galaxy has a relatively smooth appearance, though subtle features suggest ongoing or recent interactions with another galaxy. 
