The galaxy appears to be a relatively smooth, elliptical galaxy with an apparent red shift. The light distribution suggests a dominant bulge component with little or no visible disk. It exhibits a concentrated central region with a gradual decrease in surface brightness outwards. The color is predominantly yellow, with some hints of redder and bluer regions. The redder regions may indicate areas of older stellar populations or dust obscuration, while the bluer regions may point to younger stars, but these are very faint and poorly defined. There is no clear evidence of spiral arms or strong star formation regions. The overall morphology suggests an evolved system with a relatively low star formation rate. There is no apparent presence of any tidal features or signs of ongoing merging activity. It appears to be a relatively isolated galaxy.
