The galaxy presents a somewhat diffuse, non-distinct morphology, likely a spiral or irregular galaxy. The central region appears slightly more concentrated, suggesting the presence of a bulge, though it is not sharply defined. The galaxy displays a subtle disk-like structure, but the arms, if present, are not well-defined or tightly wound. The color profile indicates a blueish tint, particularly in the outer regions, suggesting the presence of younger stars. A small amount of reddish areas throughout the galaxy might suggest areas of dust or older stars. Overall, the galaxy appears to be a low-mass system, undergoing some degree of star formation. There might be some interaction occurring as the structure is not completely regular.
