The galaxy presents as a largely smooth, elliptical-like structure. Its overall color is slightly red, indicative of an older stellar population. The core region exhibits a brighter, yellowish hue, which may suggest a concentration of older stars. There is very little evidence of spiral arms or distinct disk features in the image. The galaxy appears generally undisturbed, showing no significant signs of a major merger. Minor distortions can be observed. Based on the color indices, the galaxy may have had some star formation activity in the past.