This galaxy presents as an elliptical morphology. It exhibits a bright, concentrated central bulge, which appears to be composed of older stellar populations, judging from its yellow to white hue. The galaxy appears relatively smooth in texture, with a high degree of central concentration. There are no clearly defined spiral arms, suggesting the absence of significant ongoing star formation. The outer regions of the galaxy show a gradual decrease in luminosity, fading into the background sky. Minor irregularities are present in the outer halo, perhaps indicative of past interactions or minor disturbances. The shape is somewhat elongated, displaying an aspect ratio that suggests it is not a perfect sphere but rather has some degree of ellipticity. The galaxy is moderately distant, indicated by the redshift. 
