This galaxy exhibits a generally smooth morphology, appearing elliptical in shape. It possesses a central bulge that is more luminous than its surrounding regions. This central region displays a distinct orange hue suggesting an older stellar population. The outer regions are fainter, with hints of a bluer color. The general lack of defined spiral arms suggests a classification towards the early-type end of the Hubble sequence, and the lack of any major distortions or tidal features implies it has not undergone a major merger recently. There is a slight elongation to the galaxy's profile, however, the roundness fraction suggests the morphology has an elliptical nature to it. Some indications suggest minor disturbances or interactions may have occurred in the past.
