The galaxy appears to be a somewhat elongated or cigar-shaped system. The central region displays a concentrated brightness, indicative of a possible bulge. There is a noticeable color gradient across the galaxy, with a more reddish hue dominating. This color suggests an older stellar population and a lower rate of ongoing star formation. There is a faint disk structure that has a more apparent golden hue, though difficult to resolve with high fidelity, possibly due to the viewing angle or the limits of the image resolution. There appears to be no signs of major mergers occurring but minor disturbances cannot be ruled out. 
