The galaxy appears as a relatively compact object, approximately circular in projection. The central region exhibits a bright, smooth appearance, suggesting a dominant bulge component. There is a faint hint of a disk structure or feature extending from the central bulge, but it appears subtle, potentially masked by the brightness of the bulge.

The color gradient shows a bluer hue in the core, becoming redder towards the edges, possibly indicating older stellar populations in the outer regions. There is some noticeable disturbance in the morphology of the galaxy, likely due to a merger event. This event might be interacting tidally with the main body, causing the faint features. The system seems to be undergoing some form of interaction, potentially influencing its shape.
