The galaxy appears as a centrally concentrated, elliptical-like structure. The light distribution is relatively smooth, with a general lack of distinct features such as spiral arms or prominent dust lanes. There is a subtle color gradient, with a slightly bluer hue towards the outer regions and a yellow/red hue toward the core. The galaxy shows a lack of significant ongoing star formation, but hints of activity are seen. The overall morphology suggests that the galaxy is a relatively evolved system, possibly an elliptical galaxy transitioning to a lenticular, but could potentially be a spiral system being viewed directly on. Some distortion may be visible, which is an indicator of a past merger event.