The galaxy presents as a centrally concentrated, elliptical or lenticular morphology. A significant bulge component dominates the central region, exhibiting a yellowish hue indicative of an older stellar population. There is some evidence of a disk component, but it appears relatively smooth. There are no apparent spiral arms. The surrounding halo appears relatively smooth. The overall color gradient suggests ongoing, albeit low, levels of star formation. There is a very slight indication of a possible gravitational interaction with another galaxy to the left, which would explain the minor level of ongoing star formation.
