The galaxy presents a largely smooth, elliptical morphology. It is relatively compact, with a concentrated central bulge that graduates outward in luminosity. The color profile suggests a predominantly older stellar population, with a yellowish-red hue dominating the core and inner regions, trending towards slightly bluer tints on the outer edges. There is no obvious spiral arm structure or dust lane obscuration visible. The overall appearance indicates a gravitationally settled system with minimal ongoing merger activity or major tidal disturbances. The moderate redshift suggests that this galaxy is relatively distant. The blue tinges at the edge suggest possible star formation, but this is limited. Based on its color and morphology, it is likely an elliptical galaxy.
