The galaxy presents as a roughly elliptical shape, with a high degree of central concentration. It exhibits a smooth, relatively featureless morphology, lacking prominent spiral arms or other distinct structural components typically seen in disk galaxies. The galaxy's color profile appears to be dominated by yellowish-orange hues, suggesting a stellar population primarily composed of older, redder stars. Some disturbances may be present, though none are prominent, indicating a possibly ongoing, or recent, minor interaction with another galaxy. The estimated size and luminosity place it within the range of a massive galaxy, exhibiting relatively moderate star formation. Its specific star formation rate indicates that the star formation rate is low in proportion to its stellar mass. The galaxy's overall appearance suggests a relatively evolved system nearing the later stages of its evolution.
