The galaxy presents as a relatively smooth, elliptical structure. The central bulge exhibits a yellowish-white hue, suggesting a population of older, less massive stars. The outer regions appear bluer, potentially indicating the presence of younger stars and ongoing star formation, although this is not pronounced. There is a slight elongation visible, giving it a somewhat cigar-like shape rather than a perfectly spherical appearance. No distinct spiral arm structures are discernible, nor are there any obvious signs of recent or ongoing major mergers or tidal disturbances. The galaxy appears relatively isolated and undisturbed. Overall, the morphology suggests a mature galaxy with a mix of stellar populations and a moderate level of star formation.
