The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology with little evidence of spiral arms or a disk structure. Its color index suggests a population of older stars. The galaxy shows a high degree of central concentration. It seems to be fairly isolated with no signs of significant interaction or ongoing merger activity. The galaxy has an estimated effective radius (half-light radius) of approximately 5 kpc. The galaxy is receding from us at a significant fraction of the speed of light, as indicated by its redshift. This suggests a considerable luminosity. Based on the color, it is possibly experiencing low levels of on-going star formation.
