The galaxy presents as a relatively smooth, elliptical structure. It exhibits a moderate degree of elongation, appearing somewhat cigar-shaped rather than perfectly round. There is a distinct central bulge, which appears to be yellowish-white, suggesting an older stellar population. The outer regions of the galaxy show a subtle bluish hue, potentially indicating the presence of younger stars, although the contribution seems minimal. No prominent spiral arms or significant dust lanes are discernible. Overall, the galaxy's morphology suggests an evolved system with a relatively low rate of ongoing star formation, presenting a smooth, undisturbed appearance.
