The galaxy presents as a slightly elongated structure with a noticeable color gradient. There is a brighter, bluer region at what appears to be one end, gradually transitioning to a redder, more diffuse region at the opposite end. The morphology is neither perfectly smooth nor exhibiting grand spiral arms, and it shows some signs of disturbances, potentially indicative of a past or ongoing interaction. The galaxy's shape is more akin to an intermediate form, with a slightly flattened but not fully disk-like appearance. There may be an ongoing merger or tidal interaction with a nearby companion.
