The galaxy presents as a somewhat elliptical, relatively smooth and centrally concentrated luminous object. The core exhibits a bright, yellowish hue, suggesting an older stellar population. Moving outward from the core, the galaxy appears more diffuse, displaying a gradual decrease in surface brightness. There's a slight elongation visible, indicating a deviation from perfect circularity. Faint, subtle irregularities can be discerned in the outer regions, potentially suggestive of minor disturbances or tidal interactions. The overall color profile indicates a galaxy with a dominant population of evolved stars, with subdued indications of ongoing star formation.
