This galaxy appears to be an interacting system, possibly in the early stages of a merger. The primary component presents a somewhat smooth morphology, with a slightly elongated, disk-like structure. A distinct, bluer region is observed within this main body, potentially indicative of ongoing star formation. The bluer color suggests a population of younger, hotter stars. A secondary, smaller galaxy lies nearby, displaying a more diffuse and irregular form. It shows a slight tidal disturbance that supports an interaction. There is some redness in the main body, suggesting a relatively older population of stars. The galaxy exhibits characteristics consistent with a moderate mass and an active, albeit not exceptionally high, rate of star formation. The overall shape is somewhere between round and elongated, and the system may have some degree of tidal distortion.
