The galaxy presents a generally smooth and rounded morphology. Its central region exhibits a significantly higher concentration of light, appearing bright and yellowish-white, suggesting a population of older stars. The light then fades to a less saturated red color. The outer regions of the galaxy diffuse outwards in a roughly spherical shape, with a lower surface brightness. There is no evidence of prominent spiral arms or a well-defined disk component. The galaxy does not appear to be strongly interacting or merging with any other galaxies. The overall structure suggests an early-type galaxy with no significant dust lanes. There is no significant amount of blue light, therefore, it does not have a very high rate of star formation.
