This galaxy appears to be a relatively smooth, elliptical galaxy, although some minor disturbances are possibly present. It presents as somewhat elongated rather than perfectly spherical. The central region exhibits a higher concentration of light, indicating a prominent nucleus. The overall color profile suggests a population of older stars, with a slight bluer component in the extended regions. The lack of distinct spiral arms or dust lanes supports the classification as an elliptical type. There is a subtle asymmetry in the outer regions, potentially indicating a past interaction or minor merger event. The galaxy does not show signs of significant ongoing star formation.
