The galaxy presents as an elliptical morphology, appearing largely smooth and centrally concentrated. It exhibits a generally round shape, showing little deviation from circularity. There is no evidence of significant tidal disturbances or ongoing major mergers, though subtle irregularities might suggest minor gravitational interactions. The galaxy displays a color gradient, with a bluer hue apparent in the outer regions that transitions to a redder central core, indicative of variations in stellar populations and dust distribution. It shows a degree of star formation activity, which may be concentrated in specific regions or contributing to the diffuse blue glow observed. Overall, this galaxy appears to be a relatively undisturbed, mature system with a mix of stellar populations and a moderate level of ongoing star formation.
