The galaxy presents as a relatively compact object. It appears to be either a close binary galaxy system or a galaxy that is currently undergoing a merger. The morphology suggests two distinct, bright central regions that are separated by a small distance, indicating a possible interaction. There is a slight asymmetry in the overall shape, possibly from gravitational disturbances. The colours appear smooth and generally uniform, suggesting the presence of older stellar populations, though bluer hues are seen near the outer edges of the two centers indicating some star formation. There is no sign of a prominent disk structure. Overall, the galaxy's structure is somewhat amorphous, with some signs of disruption.
