The observed galaxy appears as a relatively smooth, elliptical-like structure. The light distribution suggests a high degree of central concentration. There is no strong evidence of distinct spiral arms or a prominent bar. The galaxy appears largely featureless, with a subtle color gradient transitioning from a slightly bluer core to redder outer regions. This color variation could indicate ongoing star formation in the central regions, although the overall smoothness suggests that star formation is not a dominant process at the present time. The roundness of the galaxy is fairly high, with the overall shape not showing a flattened disk or a highly elongated structure. There's no obvious sign of significant tidal disturbances or recent merger activity affecting the morphology of this galaxy.
