The galaxy presents as a single, dominant, and relatively smooth light source. It exhibits an elliptical morphology, appearing nearly circular in projection with subtle variations in color temperature across its surface. The central region displays a higher concentration of yellow light, suggesting an older stellar population. There is a lack of clear spiral arm structure or significant dust lanes. The galaxy has a well-defined edge, indicating it is not currently undergoing a major merger event. The image suggests the galaxy is primarily supported by random motions rather than rotation. Overall, the galaxy appears to be a quiescent system with little ongoing star formation.
