The galaxy appears to be a relatively luminous elliptical galaxy at a redshift of approximately 0.25. It exhibits a smooth, centralized light distribution with a high degree of radial symmetry, suggesting a lack of significant spiral arm structure. The central region is significantly brighter, indicating a dense concentration of stars, likely an older stellar population. There is no apparent dust lane or active galactic nucleus. There is very little evidence of tidal disturbances, implying that it has undergone only minor merging events in the past. The elliptical shape suggests that it is a dynamically relaxed system.
