The galaxy presents as a relatively smooth, centrally concentrated object, lacking a well-defined spiral structure or prominent dust lanes. The primary body of the galaxy exhibits a diffuse, elliptical morphology. The color gradient suggests a somewhat older stellar population, transitioning from a slightly bluer hue near the core to redder hues in the outer regions. Overall, the galaxy appears to be an elliptical system undergoing a relatively low rate of star formation. There is the possibility of minor tidal disturbance based on some asymmetries.