The galaxy appears as a single, concentrated body with a smooth morphology. The color profile suggests a dominant older stellar population, exhibiting a reddish hue overall. The galaxy appears mostly uniform in color and brightness, lacking any obvious spiral arm structures or distinct features. The shape is generally round, with a slight deviation from perfect circularity. The object shows evidence of possible interactions or disturbances. There are no clear signs of a prominent central bulge or active galactic nucleus. The light is fairly concentrated suggesting some degree of established structure and gravitational binding. Based on the apparent magnitude and color, the galaxy appears to be a relatively massive and luminous object. Overall, the galaxy is most likely an elliptical galaxy with a significant fraction of old stars.
