The galaxy presents a predominantly smooth and rounded morphology, characteristic of an elliptical or lenticular galaxy. It exhibits a concentrated central bulge, which dominates the overall light profile. The light emitted from the galaxy skews toward the redder end of the spectrum, suggesting an older stellar population. The galaxy shows a relatively high luminosity, suggesting a higher than average stellar mass. There is little evidence of recent or ongoing star formation, supported by the galaxy's red color. A very slight disturbance can be seen on the left edge of the object, though this could be due to lensing of other objects nearby.
