The galaxy appears to be an irregular system, exhibiting a somewhat disturbed morphology. There is evidence of a central, more concentrated region that has a smoother appearance to it. A prominent extended feature curves outwards from this central region, possibly indicative of tidal interactions or a disrupted disk. The color distribution shows variations, with a mix of bluer and redder regions within the galaxy. The bluer regions are concentrated in the outer feature, suggesting ongoing star formation. Redder regions are more prominent in the center, which may indicate an older stellar population, dust extinction, or redshift. The galaxy does not present a clear spiral or elliptical structure, leaning towards a more amorphous, interacting classification. Evidence suggests this galaxy may be a merger or undergoing significant gravitational interaction. 
