The galaxy presents as a largely smooth, elliptical-type morphology, with a high degree of central concentration. The light distribution suggests a well-defined spheroidal component, with a radially decreasing surface brightness profile. There is no obvious evidence of spiral arm structure or a prominent disk. The overall color appears relatively uniform and somewhat red-shifted, suggestive of an older stellar population and lower levels of ongoing star formation. Minimal signs of tidal disturbance or recent merger activity are visible.
