The galaxy presents a somewhat amorphous structure, appearing neither purely elliptical nor a well-defined spiral. It exhibits a generally smooth profile with a moderate concentration of light towards the center. The shape is close to circular. Some subtle irregularities or minor disturbances may be present in its morphology, potentially indicative of past interactions. Patches of redder emission suggest the presence of older stellar populations, while green hues are spread throughout the galaxy, possibly related to ionized gas or ongoing star formation. There is some possible merging, with some disturbance to the shape of the main part of the galaxy.
