The galaxy appears as a centrally concentrated, smooth object, exhibiting a roughly elliptical morphology. There is a general lack of defined spiral arm structure or significant dust lanes visible at this resolution. The color profile suggests a dominant population of older stars, as indicated by the yellow-orange hue, which is characteristic of evolved stellar populations. While the object appears mostly undisturbed, there is a possible indication of minor asymmetry in its outer regions, potentially hinting at a past interaction or minor disturbance event. Overall, this appears to be a relatively massive galaxy with low star formation.
