The galaxy appears as an elliptical-shaped entity, exhibiting a smooth, featureless morphology with no discernable spiral arms or distinct substructures. Its light profile suggests a centrally concentrated brightness distribution, gradually diminishing toward the outer edges. The color is relatively uniform across the galaxy, showing a bias towards redder wavelengths. This redder hue implies an older stellar population, potentially indicating a lower rate of current star formation. The galaxy's axial ratio indicates a moderate elongation, suggesting a deviation from a perfectly circular shape, and an inclination relative to our line of sight. The overall impression is of a mature, quiescent galaxy with a predominantly evolved stellar population.
