The galaxy presents as a smooth, centrally concentrated object, displaying an elliptical morphology. The light distribution appears relatively uniform with a lack of distinct spiral arms or prominent features suggesting recent major merger activity. The color gradient indicates a population of older stars, with a yellowish-red hue dominating the galactic nucleus, suggesting minimal on-going star formation within the central region. The outer regions show a slightly bluer tint, suggesting the presence of some younger stars in those areas. There is a hint of a tidal tail present at the edges of the galaxy, suggesting there was a minor merger or galactic disturbance. Overall, the galaxy appears to be a relatively relaxed system, primarily composed of aging stars and with a low rate of current star formation.
