The galaxy appears to be an elliptical galaxy, elongated in shape. Its central region exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions transition towards a bluer color, suggesting the presence of younger, hotter stars. The overall structure is relatively smooth with no distinct spiral arms or significant dust lanes visible. There are hints of a slight disturbance in the morphology, such as a subtle warping of the disk or faint tidal features, indicating a possible past or ongoing minor interaction with another galaxy. However, the galaxy seems generally undisturbed. Overall, the galaxy has characteristics consistent with an elliptical galaxy undergoing slow, consistent star formation.
