The galaxy presents a somewhat irregular morphology. A central bulge region is apparent, appearing relatively bright and concentrated, exhibiting a yellowish-white hue. Extending from this central region are fainter, somewhat diffuse structures. One side exhibits a bluish tint, suggesting the presence of younger stars or active star formation regions. Conversely, the opposite side exhibits a more reddish hue, potentially indicating the presence of older stellar populations or dust obscuration. There are slight visual disturbances or asymmetries in the overall structure, possibly indicative of past or ongoing interactions with another galaxy, with no large visible companion galaxy. There may be a higher rate of star formation happening, or perhaps the galaxy has undergone some sort of change due to its environment. The galaxy appears to be moderately distant, with a discernible but not highly detailed structure.
