The galaxy presents an elliptical morphology, appearing elongated in shape with a smooth, diffuse light distribution. The central region exhibits a concentrated luminosity, suggesting a high stellar density likely dominated by an older stellar population. A color gradient is observed, with a yellowish hue dominating the core, transitioning to a slightly bluer tinge in the outer regions. This could indicate ongoing, though subdued, star formation activity in the outskirts. No spiral arm structures or prominent dust lanes are discernible. The overall appearance suggests a relatively evolved system with a substantial mass. There's no strong evidence of any major recent merger events or significant tidal distortions.
