The galaxy presents as a smooth, elliptical form, with a slight elongation. The central region exhibits a bright, concentrated luminosity, indicative of a substantial stellar population. Moving outward from the core, the light gradually diminishes. There is a subtle color gradient, with the inner region showing a yellowish hue, transitioning to bluer tones in the outer areas. No distinct spiral arms or prominent dust lanes are discernible. The overall morphology suggests an evolved system with a relatively high degree of symmetry. Slight disturbances may be present.