The galaxy presents a complex morphology. It appears to be a spiral galaxy, seen at an oblique angle. The central bulge is not clearly defined, and there are faint hints of spiral arm structure, though the arms are not well-defined or continuous. The galaxy exhibits a blueish hue in certain regions, suggestive of ongoing star formation. There is also a redder component of the galaxy, towards the center, which suggests an older stellar population. There appears to be some indication of tidal interaction and/or minor disturbances in the galaxy's morphology, possibly indicating a recent or ongoing merger event. Overall, the structure is disturbed with asymmetry, and indistinct features. The outer regions of the galaxy show faint extensions, that may be the remains of a tidal tail, further supporting the notion of a past merger.