The observed galaxy presents a predominantly smooth morphology, characteristic of an elliptical galaxy type. It appears well-defined with a concentrated central bulge that emits a significant amount of light. The light gradually diminishes outward with no prominent spiral arm structures or distinct features discernible. The central region exhibits a yellowish hue which likely indicates an older stellar population, while the outer edges seem slightly bluer in color implying a smaller population of younger stars. There is no evidence of recent or ongoing major merging events or significant disturbances, and it exhibits a generally elliptical shape.
