This galaxy appears to be a relatively smooth and concentrated system. The central region exhibits a reddish hue, potentially indicating an older stellar population or significant dust obscuration. Surrounding this core, a slightly bluer, more diffuse halo is observed, suggesting the presence of younger stars or a population with less dust extinction. The galaxy displays a mildly elliptical shape, with a ratio of major to minor axes indicating a relatively low degree of flattening. Some subtle disturbances are visible, such as asymmetric light distribution in the halo. These features suggest a possible past interaction or minor merger event. Overall, the galaxy is not strongly star-forming, but shows some level of star formation in the outer regions. The luminosity is high, suggesting a massive galaxy.
