The galaxy presents a relatively smooth, elliptical morphology, appearing quite round in shape. There is a subtle elongation and some diffuse light extending from the main body, however no obvious signs of spiral arms or a prominent disk structure are visible. The light profile suggests a concentration of older stars, indicated by the reddish hue in the galaxy's core, with a faint blue halo surrounding it suggesting a bit of ongoing star formation. It shows no major disturbances, although there is evidence of a potential minor disturbance in the outer regions, based on some asymmetry in the light distribution. Overall, this galaxy is likely a massive system with a considerable stellar mass, but with a relatively low rate of star formation. The distance to the galaxy, as indicated by its redshift, confirms that it is an extragalactic object.
