The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a distinct yellowish-orange hue, suggesting a population of older stars with lower star formation activity. The overall shape is largely circular. There is no prominent disk structure. The smoothness of the light distribution indicates the absence of major disturbances or merging events. There might be very subtle indications of minor irregularities, but the light is concentrated in the core of the galaxy.
