The galaxy presents as a primarily smooth, elliptical-like structure. A bright, concentrated central bulge dominates the core. This core exhibits a yellow hue, likely indicating an older stellar population. Surrounding the central bulge is a fainter, more diffuse halo that has a bluer tint relative to the center. The light distribution suggests a high degree of central concentration. No distinct spiral arm structures or significant dust lanes are visible in this image. The galaxy appears relatively isolated with no signs of major merging activity or tidal disturbances. The shape is slightly elongated, deviating minimally from a perfect circular form. Overall, it appears to be a relatively massive galaxy exhibiting moderate star formation.
