The galaxy presents as an elliptical or lenticular type, with a generally smooth morphology and a high degree of central concentration. The overall color is relatively red, suggesting an older stellar population. There is some evidence of bluer regions, possibly indicating regions of recent or ongoing star formation. The isophotes are generally round, though there is some irregularity to the shape. There appears to be a minor disturbance in the morphology, likely due to interaction with a smaller galaxy. There is no clear evidence of a prominent disk or spiral arm structure. Overall, the galaxy appears to be a relatively massive system with a moderate star formation rate.
