The galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated light distribution. It exhibits a nearly spherical morphology, displaying a lack of prominent spiral arms or a well-defined disk structure. The color profile suggests a dominant population of older stars, giving it a yellowish hue in the central regions. There is no indication of any major ongoing merging events or significant tidal disturbances. However, there are minor asymmetries present, indicating that a minor disturbance in the past is possible. The size suggests that it's likely a large, mature galaxy.
