The galaxy presents as a single, concentrated object with a smooth, elliptical morphology. The core region exhibits a bright, yellowish-white glow, indicative of a higher concentration of older stellar populations. Moving outwards from the core, the color transitions towards a redder hue before fading into the background. A faint, diffuse halo surrounds the galaxy, lacking any prominent spiral arms or distinct features. This suggests the galaxy is likely an elliptical galaxy with little to no ongoing star formation. Any disturbances in the overall shape are minimal, implying that it has not undergone any significant merging events recently. 
