The galaxy presents a somewhat elongated morphology, appearing cigar-shaped rather than perfectly spherical. The central region exhibits a brighter, smoother appearance, suggesting a concentration of older stellar populations. Fainter, bluer regions are visible at the periphery, indicating areas of ongoing star formation. There are some faint signs of a possible disk-like structure, or faint spiral arms, but it may also just be an artifact of the imaging. It doesn't seem to have a distinct spiral structure or obvious merging activity.
