The galaxy presents as a centrally concentrated, smooth object with a generally elliptical morphology. Its color is predominantly yellowish-orange. There is no discernible fine structure such as spiral arms or a prominent dust lane. The observed light appears to be dominated by older stellar populations, with minimal evidence of ongoing star formation. The galaxy exhibits a high degree of central concentration, as expected from an object with a high mass content. The observed features suggest a well-evolved system, likely an elliptical or lenticular galaxy. There is no evidence of tidal features, strong gravitational lensing, or other obvious interactions with companion galaxies, indicating that the galaxy is relatively isolated.
