The galaxy presents as a slightly elliptical, disk-like structure with a smooth, concentrated bulge. The galaxy exhibits a color gradient, appearing more yellow/orange toward the core, suggesting a higher concentration of older stars. The outer regions of the disk display a bluer hue, potentially indicating more recent star formation. There is no strong evidence of spiral arm structure or significant dust lanes visible. The overall appearance suggests a galaxy undergoing a transition from a more actively star-forming state to a more quiescent state. No obvious signs of major mergers or tidal disturbances are immediately apparent. The galaxy is relatively isolated.
