The observed galaxy presents as a somewhat elongated structure. Its morphology appears to be largely smooth, though subtle irregularities suggest the possibility of underlying features. The galaxy exhibits a color gradient, transitioning from a slightly bluer hue in its central region to redder tones towards its outer edges. This could be indicative of differing stellar populations or dust distribution within the galaxy. There is no clear evidence of spiral arms or a prominent disk. Subtle distortions are present along the galaxy's periphery which suggests possible interactions with other galactic bodies. The galaxy's overall light distribution is centrally concentrated, gradually decreasing in intensity with increasing distance from the core.
