The galaxy presents as a relatively compact object. Its overall morphology appears disturbed, with some irregular features and a hint of asymmetry in its shape. The central region seems to be brighter than the outer regions. There is some faint structure suggesting either faint spiral arms or tidal features caused by a minor disturbance, possibly a past or ongoing interaction with a smaller object. There may be some low-level star formation activity, particularly in the areas of potential distortion.
