The galaxy presents as a relatively smooth, elliptical object with a high degree of central concentration. There is a distinct yellow-orange hue to the core, suggesting a population of older stars. Fainter, diffuse green-blue emission is observed in the surrounding regions, possibly indicating ongoing, albeit subdued, star formation activity. The overall morphology suggests a system that has largely completed its primary evolutionary phase. There is potential evidence of minor tidal disturbances or interactions present, given the asymmetry in the outer halo, which indicates recent or ongoing accretion events. It is also possible the galaxy is in the process of merging with another galaxy.
