The galaxy presents as an elliptical morphology, appearing largely smooth and well-defined. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The color profile indicates an older stellar population, predominantly yellow-red hues, indicative of evolved stars. There is no apparent dust lane or spiral arm structure visible in this image. The galaxy displays high degree of rotational symmetry, suggesting it is likely a relatively relaxed system. There is no indication of recent mergers or significant tidal interactions. The overall appearance suggests a massive galaxy, potentially at intermediate redshift. Its star formation rate is likely low.
