The galaxy presents as a diffuse, irregular object. Its overall morphology is suggestive of a disturbed system, potentially undergoing a merger or exhibiting signs of past gravitational interactions. The light distribution across the galaxy is uneven, with a noticeable central concentration of light that may represent the galactic core, although it is not sharply defined. 

There appears to be faint tidal features or extended stellar streams emerging from the main body of the galaxy, suggesting a potential ongoing or recent merger event. The color of the galaxy indicates a mixture of stellar populations, with some regions appearing bluer, possibly indicative of recent star formation, and others appearing redder, which may represent older stellar populations. The lack of a prominent disk-like structure further supports the classification as an irregular or disturbed galaxy.
