The galaxy appears to be a moderately luminous system at a redshift of approximately 0.1, suggesting a considerable distance. Morphologically, it exhibits characteristics of a relatively smooth galaxy, yet there is a hint of either a disk-like structure or some form of internal feature disrupting complete uniformity. The dominant shape is largely round, with a suggestion of intermediate ellipticity. There are indications of possible gravitational interaction or recent merger activity. The overall color suggests a population of older stars. This galaxy is likely a relatively massive system with moderate star formation activity.
