This galaxy appears to be a relatively smooth, centrally concentrated object. It has a roughly elliptical shape, appearing more elongated than perfectly circular. There is a subtle color gradient visible, with a slightly bluer core region fading to redder hues in the outer regions of the galaxy. There is no evidence of a strong central bulge or distinct spiral arms. The overall morphology suggests a system that is not undergoing major interactions or disturbances, though there is some minor asymmetry that could indicate past gravitational interactions. The galaxy exhibits relatively low star formation activity and is likely composed primarily of older stellar populations.
