The galaxy presents a generally smooth, elliptical morphology with high degree of radial symmetry. The galaxy exhibits a concentrated central bulge with a gradual decline in luminosity towards the outer regions. The color is predominantly yellowish-orange across the observed spectrum, indicative of an older stellar population with lower ongoing star formation. There is no prominent dust lane visible, and no clear spiral arm structure is discernible. There is a slight elongation to the morphology but it is generally circular in appearance. Any signs of tidal disturbances or mergers are subtle, if present at all.
