The galaxy presents as a somewhat elongated, cigar-shaped structure. Its central region exhibits a yellowish-white hue, suggesting a concentration of older stellar populations. Proceeding outwards from the core, the light gradually diffuses into a fainter bluish-white halo. The overall morphology seems relatively smooth with hints of a faint disc structure. The galaxy does not appear to be undergoing any major merging events or experiencing significant tidal disturbances. There are no discernable prominent spiral arms or dust lanes, which may indicate that star formation activity is relatively low.
