This galaxy presents as a relatively smooth, concentrated object with a slightly elliptical morphology. The central region exhibits a bright, yellowish-orange hue, suggesting a population of older stars and reduced star formation activity. The outer regions display a more diffuse, greenish coloration, potentially indicating the presence of younger stars and ongoing, albeit low, star formation. There is no clear evidence of spiral arm structures or significant dust lanes. Minor disturbances are possibly present in the outer edges, but the galaxy appears relatively isolated.
