The galaxy appears as an elongated, roughly ellipsoidal structure with a moderately bright core that fades outwards. There is a hint of structure but it appears largely homogenous. It may be undergoing or recently completed a minor disturbance or merging event based on the lack of strong symmetrical order. There is no clear dust lane, spiral arm or strong morphological feature discernible at this resolution. The object demonstrates a smoothly distributed emission profile, typical of a later-type disk galaxy or possibly an elliptical galaxy seen edge-on.
