The galaxy appears compact, exhibiting a roughly elliptical morphology. The central region displays a high surface brightness, suggesting a concentrated nucleus. There appears to be a slight asymmetry in the outer regions, possibly indicating minor gravitational interaction or internal disturbances. Color gradients are subtle, with a slightly bluer hue in one area and a slight redder hue in another area, potentially due to variations in stellar populations or dust content within the galaxy. The overall structure lacks prominent spiral arms or a well-defined disk. The absence of strong morphological features could classify this as an elliptical or lenticular galaxy.
