The galaxy appears as an elliptical or lenticular morphology, characterized by a smooth and relatively featureless profile. The light distribution is centrally concentrated, with a gradual decrease in intensity towards the outer regions. It exhibits a generally rounded shape with the exception of a small disk shape, showing some irregularity. There is a hint of redder color, indicating an older stellar population and suggesting a lower rate of ongoing star formation. The estimated size of the galaxy seems to be consistent with a moderate size. The structure is relatively undisturbed, with no obvious signs of recent or ongoing major mergers, although a slight distortion could indicate a minor disturbance.
