The galaxy appears as a centrally concentrated object with a relatively smooth morphology. There is a slight elongation to the shape, but it is largely round. The core of the galaxy exhibits a bright, almost stellar-like nucleus, fading into a surrounding diffuse halo. The overall color is a muted blue-white, suggesting the presence of a moderate population of young stars. Faint traces of redder regions can be discerned in the surrounding area, potentially indicative of older stellar populations or dust absorption. No spiral arm structures or distinct features are easily discernible. There is a faint indication of a slight disturbance in its overall shape, possibly due to a minor gravitational interaction, but there's no sign of a major ongoing merger or disruption.
