The galaxy presents as a cigar-shaped, elongated structure. A central bulge is visible, appearing smoother and more concentrated than the outer regions. There is a hint of a disk surrounding the bulge that appears thin and stretched with irregular edges. The galaxy exhibits a color gradient with a bluer tint towards the outer edges. The smooth appearance of the bulge suggests an older stellar population. There is no indication of active star formation. No major merger events are apparent. There are some minor disturbances but these are difficult to identify. The morphology is predominantly smooth.
