The galaxy presents as a smooth, elliptical morphology with a high degree of central concentration. Its color index suggests a population of older stars, emitting predominantly in the redder portion of the spectrum, with a central yellowish hue. The galaxy exhibits a slight elongation, with a ratio of approximately 3:1 between its major and minor axes, indicating a moderate degree of ellipticity. No spiral arm structures or dust lanes are discernible, contributing to its overall smooth appearance. There is no visible evidence of recent or ongoing major merger activity. Minor disturbances cannot be ruled out, but are not immediately apparent in the image. The lack of blue color indicates little current star formation. The galaxy appears relatively undisturbed and well-defined.
