The galaxy presents as a somewhat elongated, cigar-shaped structure, exhibiting a predominantly smooth morphology. A central bulge region is discernible, appearing relatively bright and concentrated. The overall color profile suggests a higher concentration of older stellar populations, though some bluer regions are present, hinting at ongoing or recent star formation activity. There is a hint of a disk structure. Patches of what seem to be areas with more intense recent or ongoing star formation are observable, with slightly reddish-orange colors. These areas of star formation appears concentrated around the center and edges. Evidence of any significant interaction or major merger is not immediately obvious, however, subtle disturbances in the shape indicates that minor disturbances have occurred.
