The galaxy presents as a predominantly smooth object with a moderate ellipticity. Its overall morphology suggests a relatively undisturbed system, lacking any obvious signs of tidal interactions or major mergers. The light profile appears centrally concentrated, transitioning smoothly outwards. The color distribution suggests a dominance of older stellar populations. The slight elongation indicates that the galaxy likely has some rotational support. Based on the smooth appearance and redder color, it's probable that star formation activity within the galaxy is currently low. No distinct spiral arms or a prominent disk are apparent in this image. The galaxy has a reddish hue, which could indicate either dust or an older population of stars.
