The galaxy presents a predominantly smooth morphology, indicative of an elliptical or lenticular type. There is little evidence of spiral arms or significant dust lanes. The overall color is a somewhat yellow hue, suggesting an older stellar population with fewer young, massive stars. The shape is quite round, with a very small deviation from circularity.

There is no obvious sign of any major ongoing merger activity or significant tidal disturbances in the immediate vicinity of the galaxy. The core appears to be centrally concentrated with a fairly gradual decrease in surface brightness outwards. The galaxy is a fairly compact object, with no extremely diffuse outer regions are apparent within the image frame. Its redshift indicates that it is relatively distant.
