The galaxy appears to be an elliptical morphology with a moderately high Sersic index, indicating a concentrated central region. Its shape is elongated, possessing a clear major and minor axis with an apparent axial ratio of approximately 0.6. The galaxy displays a smooth profile, with the vast majority of visual classification reports not showing mergers or disks. The overall color gradient suggests a population dominated by older stars, although weak blue hues are present in the nucleus. The galaxy's effective radius, encompassing half of the total light, is observed to be on the order of 3 kiloparsecs.
