The galaxy appears to be a slightly tilted disk galaxy, approximately 11 kpc in radius. The central bulge is prominent, exhibiting a yellowish-orange hue, suggestive of an older stellar population. The disk shows evidence of some structure, with hints of spiral arms or irregular features. The color of the disk appears bluer than the bulge. There may be some minor disturbances in the morphology, although the overall structure does not indicate a major merger event. The galaxy appears to have a relatively smooth overall structure. 
