The galaxy appears to be a fairly luminous system, exhibiting an elliptical or lenticular morphology. The galaxy is mostly smooth, with no prominent spiral arm structures or strong dust lanes visible. There is a slight elongation, suggesting it might be an E4-E5 elliptical, or an S0-a lenticular. There is some distortion on the left edge, indicating a possible minor disturbance. It displays a yellow-red hue, suggesting an older stellar population and a relatively low star formation rate. The system is compact and moderately concentrated.
