The galaxy presents as an elliptical morphology, appearing largely smooth with a high degree of central concentration. The color profile indicates a population of older stars, presenting with a yellowish hue in the central bulge and a slightly redder tint in the outer regions. There is no clear evidence of spiral arms or significant dust lanes, suggesting a more evolved system with a quiescent star formation rate. Its apparent roundness suggests an orientation near face-on, lacking any significant elongation or bar structures. There is a subtle, gradual decline in surface brightness from the core outwards. There are no immediately obvious signs of ongoing major mergers or significant tidal disturbances affecting its structure. Minor disturbances, while not immediately apparent in the image, cannot be entirely ruled out without more detailed analysis.
