The galaxy presents as a relatively smooth, centrally concentrated object with a moderate ellipticity. There is a bright central bulge that dominates the overall light distribution. The galaxy appears to be a yellowish hue, indicating an older stellar population. No distinct spiral arm structures are visible, but there is some indication of a faint disk. The outer regions of the galaxy fade gradually into the background, suggesting a high Sersic index, and is an oblate spheroid. There is a hint of some disturbance or minor interaction in the outer regions of the galaxy.
