The galaxy presents as a roughly elliptical structure with a bright, concentrated central bulge exhibiting a yellowish-orange hue. A disk-like component, less luminous and showing a bluish tinge, surrounds the central bulge. The outer regions of the disk appear smooth, with no obvious spiral arm structures readily discernible. The overall appearance suggests a possible transition from a more elliptical morphology towards a disk galaxy. There are no strong indicators of ongoing major merger activity, although there may be minor disturbances or asymmetries present in the faint outer regions.
