The galaxy presents as an elliptical morphology, exhibiting a smooth light distribution without obvious spiral arm structure. The object's color profile suggests a dominant population of older stars, contributing to its yellow-red hue, particularly concentrated towards the galaxy's core. The minor axis is compressed relative to the major axis, contributing to the galaxy's shape. The outskirts of the galaxy appears fainter, indicating the density of stars decreases significantly away from the center. No signs of active galactic nuclei, intense star formation regions, or merger events are apparent from this image.
