The galaxy appears as a primarily smooth, elliptical structure. Its overall color profile suggests a greater abundance of older stellar populations, with a concentration of yellow-orange hues toward the galactic center. Fainter blue regions are observed primarily around the center of the galaxy, suggesting limited but potentially ongoing star formation activity. The galaxy's shape is approximately spheroidal but leans toward in between round and cigar shaped, lacking strong spiral arm features or a well-defined disk. There is no evidence of a major ongoing merger, but it is difficult to rule out minor interactions based on this image alone. Based on light distribution, the system is moderately luminous with an approximated intermediate mass, and is located at a non-negligible redshift.