The observed galaxy presents as a roughly circular, smooth object, exhibiting a high degree of central concentration. The primary body is largely featureless, but there is a small, distinct, secondary condensation of light located peripherally to the main structure. The light distribution suggests a spheroid-like morphology with a possibly ongoing or past merger event that is close in proximity. The galaxy displays a color profile indicating intermediate wavelengths are more prominent, whereas long wavelengths are seemingly attenuated. The overall appearance implies a relatively evolved system with a potentially complex interaction history.
