The galaxy presents an elongated, cigar-shaped morphology. It appears to be relatively smooth in overall structure, with a subtle indication of a possible disk-like component or some form of internal structure. The galaxy exhibits a reddish-yellow hue, suggesting an older stellar population or significant dust obscuration. There is a slight color gradient across the galaxy, with a more bluish center and a redder periphery. This could potentially indicate ongoing star formation in the core. There's no clear evidence of a major ongoing merger, although some minor disturbances or tidal features cannot be entirely ruled out based on this image alone. The galaxy displays a moderate size. 
