The galaxy appears to be a relatively compact, luminous object. A central bulge dominates the structure, exhibiting a bright, concentrated core. The galaxy shows evidence of a disk component, but it is not clearly defined. There is likely some level of recent or ongoing star formation within the galaxy, suggested by the overall color, but it is not strongly indicated. Based on its apparent morphology and size, the galaxy appears to have experienced some interaction or disturbance that has prevented the development of a well-defined spiral structure. The light distribution suggests a significant degree of rotational symmetry and a low level of star formation. 
