The galaxy presents as a centrally concentrated, elliptical morphology. It exhibits a smooth, largely featureless profile, with no discernible spiral arm structures or significant dust lanes visible in this image. The color gradient suggests a population of older stars, particularly within the concentrated nucleus, which appears a pronounced yellow. The galaxy shows a slight elongation, deviating from a perfectly circular form and tending more towards an in-between profile. There are hints of some minor disturbance or interaction, and the halo gradually fades into the background sky, indicating the outer regions are populated with older, less luminous stars. The galaxy appears to have a low star formation rate, with a high degree of smoothness, indicating it's a more evolved system.
