This galaxy exhibits a generally smooth and rounded morphology, with a bright, concentrated central bulge. The overall color gradient suggests a dominant population of older stars, appearing more yellowish-red in the central regions, possibly indicating a lack of significant recent star formation there. There is a hint of bluer color extending outward from the core, which could signify the presence of younger stellar populations in the outer regions. While appearing mostly undisturbed, subtle asymmetries in the faint outer regions could suggest minor past interactions. The galaxy lacks prominent spiral arms or a distinct disk structure as viewed in this image. Overall, it appears to be a relatively evolved system.
