The galaxy appears to be an elliptical galaxy, potentially an E4 or E5 type, with a smooth, featureless morphology. It exhibits a high degree of central concentration with a bright core that gradually diminishes in luminosity towards the outer edges. There is little evidence of spiral arms or a distinct disk structure. The light profile suggests a relatively uniform stellar population throughout the galaxy. The galaxy exhibits a slightly elongated shape, appearing 'in between' round and cigar shaped. Colors suggest the presence of older stellar populations, with a noticeable yellow-red hue in the central regions. There is no noticeable dust lane or star formation activity visible in the image, suggesting a relatively passive galaxy. No signs of a recent or ongoing merger are visually apparent. 
