The galaxy presents as a complex, diffuse object. The light is concentrated centrally, with a bright core region. The object is not characterized by spiral arms, or a bulge, but rather exhibits an irregular morphology. There is some evidence of tidal disturbances, with a faint extension of light suggesting a possible interaction or past merger event. The galaxy displays a bluer color in its central region, indicative of younger stellar populations or active star formation, surrounded by yellow/green tones which suggests aging stellar populations. There are areas of low surface brightness extending from the core, contributing to the amorphous and disturbed appearance. Overall, the galaxy presents as a likely merging system or a galaxy with a history of interactions.
