The galaxy presents as a fairly smooth and rounded structure, appearing primarily elliptical in shape. It exhibits a concentrated central bulge that emits strongly in yellowish-orange wavelengths, suggesting an older stellar population. The outer regions fade into a less defined halo, which displays a mottled, slightly bluer tinge, possibly indicating the presence of more recent star formation, though at a lower rate. There is no clear evidence of a distinct disk or spiral arms. Subtle asymmetries might hint at minor gravitational interactions or disturbances. The color profile is largely consistent across the galaxy, with a gradual shift from warmer hues in the core to cooler tones in the periphery. The overall morphology suggests a galaxy in a relatively late stage of its evolution.
