The galaxy presents as a moderately bright, elliptical morphology. The central region exhibits a smooth, featureless appearance, with a high concentration of light. This suggests an older stellar population dominates the core. There is a slight elongation; tending towards an 'in between' shape rather than perfectly round, but not particularly cigar-shaped either. A subtle color gradient is observed, transitioning from a bluer hue in the outer regions to a slightly yellower tone towards the center. This color variation could indicate ongoing or recent star formation activity in the galactic outskirts, or possibly a difference in metallicities across the galaxy. No significant signs of tidal disturbances or major mergers are readily apparent, though a minor disturbance may be present, suggesting possible past interaction with another galaxy.
