This galaxy appears to be a relatively smooth, elliptical system, exhibiting a high degree of central concentration. The core region is bright and yellowish, suggesting a population of older stars. The galaxy shows only a slight ellipticity, tending toward a nearly circular morphology. There is a faint, diffuse halo extending outwards, which appears less yellow than the central core, suggesting a bluer population of stars in the outer regions. The overall color profile indicates ongoing, but possibly declining, star formation activity. There are some subtle indications of disturbance within the galaxy's structure.
