The galaxy presents an overall morphology that is generally smooth in appearance. There's a central, bright, somewhat compact core, surrounded by a more diffuse, extended halo. The halo exhibits a noticeable green hue, indicating a potentially significant amount of ionized gas. The distribution of light appears relatively symmetrical around the central core, although there is a slight asymmetry to the right. The galaxy may be undergoing minor disturbances, as suggested by subtle irregularities within the halo. This could potentially indicate a past or ongoing minor merger event.
