The galaxy presents a primarily smooth morphology, with a slight elongation visible. Its overall color is a pale blue, suggesting the presence of younger, hotter stars and potentially ongoing star formation, although at a low rate. There is a possible slight disturbance in the structure, but it's also plausible that the structure is merely asymmetric, as opposed to an indication of a major merger or strong tidal interaction. The galaxy appears to be relatively isolated, showing no immediately apparent signs of a companion galaxy that might be contributing to tidal features. The central region is more concentrated and brighter, though without a clear distinction of a galactic bulge or nucleus in this image.
