The galaxy presents as a centrally concentrated, elliptical-like structure with a smooth, relatively featureless morphology. The light profile appears to be dominated by an older stellar population, suggested by its overall yellowish hue, concentrated in the central region. There is a subtle colour gradient with radius, indicating some degree of possible age or metallicity variation within the galaxy. The galaxy seems to be mostly isolated, with no obvious signs of major tidal disturbances or ongoing mergers, however, there is potentially a minor disturbance in the morphology. Overall, the light emitted suggests moderate mass and a reduced rate of star formation. The overall shape appears to deviate slightly from a perfect circle, being more elongated.
