The galaxy presents as a slightly elongated structure with a distinct central bulge. The core exhibits a bright, yellowish hue, suggesting a higher concentration of older stellar populations. The surrounding disk appears smoother, with a gradual transition in color from yellow to bluish-white toward the outer edges. This color gradient may indicate ongoing star formation in the disk regions. There is a very slight hint of spiral structure, although it is not well-defined, possibly due to the viewing angle, or the galaxy being of an earlier type. Overall, the galaxy appears relatively undisturbed, without any obvious signs of major mergers or significant tidal interactions.
