The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus or bulge. The light gradually diffuses outwards, with a decrease in surface brightness towards the edges. There may be a hint of a very faint disk component present. There are no prominent spiral arms or irregular structures readily apparent. There does not appear to be a strong indicator of active star formation. There is no apparent indication of tidal disruption or signs of a major merger event.
