The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated light distribution with a high degree of central concentration. The morphology is largely spheroidal, with a slight elongation noticeable. The overall color is indicative of an older stellar population, showing a reddish hue. There is no clear evidence of significant dust lanes or active star formation regions within the galaxy. There also do not appear to be any signs of recent merger activity, such as tidal tails or other major disturbances to its overall morphology.
