The galaxy presents as a relatively smooth, elliptical object with an overall rounded appearance. There is a concentration of light towards the center, suggesting a prominent galactic nucleus. The light profile appears to fade gradually outward, without any obvious sharp edges or disk-like structures. There are no apparent spiral arms or significant dust lanes visible in this image. The color of the galaxy suggests a population of older stars, with a subtle reddish hue. There is no evidence of any major ongoing mergers or significant tidal disturbances from neighboring galaxies. There is a slight suggestion of possible minor disturbance in the structure.
