The galaxy appears to be a relatively smooth, elliptical galaxy with a centrally concentrated luminosity profile. The core region exhibits a yellowish-white hue, indicating a population of older stars. There is a subtle extension of the galaxy's light beyond the core, fading into a fainter, less structured halo. The overall morphology suggests a relaxed system with minimal signs of recent merger activity or strong star formation. There is a slight asymmetry in the outer regions, though this could be due to noise in the image.
