The galaxy appears to be a spiral galaxy, but its arms are not well-defined, appearing more like broad, diffuse extensions of the central bulge. The central bulge is a bright, concentrated region, displaying a smooth, elliptical shape with a soft blue hue. 

The disk exhibits a bluer color compared to the bulge, suggesting the presence of younger, hotter stars and ongoing star formation. There are some localized knots of redder light on the outskirts and fainter regions, potentially indicating areas of older stellar populations or dust obscuration. The galaxy is somewhat elongated, appearing somewhere between round and cigar-shaped.

There is a possible minor disturbance to the upper left of the galaxy.
