The galaxy presents an elliptical morphology, appearing as a flattened spheroid. Its central region exhibits a high concentration of light, suggesting a dense stellar population, likely older stars. The outer regions appear more diffuse with a noticeable falloff in luminosity moving away from the center. The galaxy's color profile indicates a relatively evolved stellar population with a redder hue, and potentially a low rate of current star formation. There is no strong evidence of prominent spiral arms or recent major merging events. Overall, the galaxy appears to be a relatively undisturbed elliptical galaxy with a smooth structure and a dominant bulge.
