The galaxy presents as an elliptical, cigar-shaped morphology. It exhibits a smooth, featureless structure with a concentrated central bulge. Color gradients are visible, shifting from bluer hues toward the outer edges to redder hues near the galactic center. This suggests older stellar populations are more concentrated towards the center. There is no indication of active star formation regions. No merging or tidal disturbance is observed in this image. The galaxy has a moderate redshift, suggesting a significant distance.
