The object appears to be a relatively smooth galaxy with a concentrated central bulge. Its morphology is largely elliptical, exhibiting a high degree of roundness. There is little discernible disk structure or spiral arm features. The galaxy possesses a color gradient, transitioning from a yellowish-white core to a slightly bluer halo. There is no indication of strong tidal interactions or major disturbances suggesting a recent merger event. The overall appearance suggests a mature system with a significant population of older stars. The galaxy is likely undergoing moderate star formation, although the lack of prominent blue regions suggests that the star formation rate is not exceedingly high.
