The galaxy presents as a disk galaxy with a dominant central bulge. The bulge exhibits a smooth, concentrated distribution of light, appearing a yellowish hue, suggestive of an older stellar population.  Extending outward from the bulge is a disk component. The disk shows a faint bluer tint in some areas, indicating pockets of younger star formation. The disk is not perfectly face-on, but rather slightly inclined to our line of sight. No strong spiral arm structure is immediately apparent, instead the disk exhibits a more diffuse appearance.  There are some areas which appear more disturbed or clumpy than others. The galaxy shows a slight elongation, but generally appears fairly circular.  The overall morphology suggests a system that is not currently undergoing any major merger activity, though there is a minor disturbance in the disk.
