The galaxy presents an elliptical morphology, with a smooth, diffuse light distribution that suggests an evolved stellar population. Its shape is generally rounded, lacking a distinct disk or spiral arms. The color gradient indicates a concentration of older, redder stars toward the core, while some subtle, bluer regions may suggest ongoing or recent star formation, particularly at the edges of the galaxy. There is a nearby object which may be interacting with the main galaxy, causing some disruption. Overall, the galaxy appears to be a relatively massive system with a quiescent star formation rate.
