The galaxy appears as a centrally concentrated object with an overall smooth morphology. There is a subtle elongation, but it generally presents as a rounded form. The color gradient indicates a redder core, potentially indicative of an older stellar population, which fades into a bluer halo region. There are no obvious spiral arm structures or dust lanes visible at this resolution, suggesting it may be a lenticular or elliptical type galaxy. Faint disturbances and features are present, indicating a potential ongoing or past interaction with another galaxy, although a merger is not immediately apparent.
