The galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology. The light distribution is concentrated towards the center, suggesting a dense core. The overall shape is largely spherical, with minimal deviation from roundness. There is no apparent disk structure or spiral arm features visible. No significant signs of ongoing or recent major merger events are detected, although a minor disturbance cannot be ruled out at this resolution. The color index suggests a population of older stars.
