The observed galaxy presents a roughly elliptical morphology, appearing largely smooth with a high degree of central concentration. The light profile suggests a fairly homogenous structure with minimal discernible features such as spiral arms or distinct dust lanes. A slight elongation is perceptible, but the galaxy approaches a circular shape. There is little to no evidence of significant tidal disturbances or ongoing merger activity, its form appears stable and relaxed. Color gradients are subtle, exhibiting a gradual shift, with the core seemingly a slightly different hue than the outer regions, suggesting variations in stellar population or composition. Light appears to be dominated by green emission, which may indicate a high redshift. Overall, the galaxy exhibits characteristics consistent with an early-type, likely elliptical, galaxy.
