The galaxy appears to be a relatively smooth, elliptical galaxy with a dominant spheroidal component. The light is concentrated towards the center, with a gradual decrease in surface brightness outward. There is little evidence of spiral arms or a prominent disk. The color profile suggests a population of older stars, with a yellowish hue dominating the central region. Faint reddish patches indicate the presence of some dust or regions of recent, albeit subdued, star formation. The morphology is generally regular, lacking signs of major disturbances or ongoing mergers, although there is a hint of minor asymmetry. The galaxy's overall structure suggests it is a mature system, likely having undergone significant dynamical relaxation.
