The galaxy presents as an elliptical morphology, appearing predominantly smooth with a slight elongation. It exhibits a concentration of light towards the center, suggesting a significant bulge component. The color appears to be a yellow-orange hue, which may indicate an older stellar population with lower ongoing star formation. There is no clear indication of prominent spiral arms or a well-defined disk. The galaxy doesn't seem to be undergoing any major merging events or significant tidal disturbances. The overall light distribution appears relatively even and undisturbed.
