The galaxy presents as an elliptical-like structure, exhibiting a smooth, centrally concentrated morphology. There appears to be little to no evidence of spiral arms or a prominent disk. The color gradient suggests a possible composition of older stellar populations. The galaxy displays a relatively high degree of roundness, with minimal deviation from a circular appearance. No significant morphological disturbances or ongoing merging activity are discernible. Overall, the galaxy appears as an evolved system, potentially a lenticular or elliptical galaxy.
