The galaxy appears to be undergoing a significant gravitational interaction, possibly a merger. The morphology presents as disturbed, with an asymmetrical distribution of light. Two distinct, luminous concentrations are observed, which may represent the cores of the interacting galaxies or significant areas of star formation triggered by the interaction. A faint, diffuse tidal tail or bridge of material extends away from the main body of the galaxy, indicative of gravitational disruption. The overall color suggests a mixed stellar population, with a central yellowish concentration possibly indicating older stars, and bluer regions within the tails suggesting ongoing star formation. There is evidence of dust lanes or obscured regions within the galaxy.
