The galaxy presents as a flattened, disk-like structure, exhibiting a prominent central bulge that appears a warm yellow-orange hue. The disk itself shows a gradient of color, with an inner region sharing the warm tones of the bulge, gradually transitioning to a bluer hue toward the outer edges. The overall morphology is relatively smooth with a slight elongation, appearing somewhat cigar-shaped. There is a suggestion of some minor disturbances or asymmetries in the disk. No distinct spiral arm structure is readily apparent. The galaxy appears to be in a relatively isolated state, showing no signs of a major ongoing merger or significant tidal interactions.
