This galaxy presents as a roughly elliptical structure with a smooth, centralized concentration of light. The core exhibits a bright, yellowish-orange hue. The surrounding halo appears fainter, displaying a subtle transition to a greenish-blue tint, suggesting the presence of a cooler stellar population and potentially some ongoing star formation, though the overall star formation rate appears low. The galaxy's overall morphology suggests a relatively mature system that is slowly evolving. There is no distinct spiral arm structure, and no strong evidence of tidal interactions or recent major mergers, though subtle irregularities in the outer regions cannot be ruled out. The galaxy appears somewhat elongated, but not to a degree that would classify it as a highly flattened system.
