This galaxy presents a largely smooth, rounded morphology. It appears as a singular, centrally concentrated object with a significant fraction of its light emanating from a bright core. There are no apparent spiral arm structures or other distinct disk features readily visible in this image. Hints of possible tidal disturbances or minor asymmetries are suggested, but they are not prominent. The color distribution across the galaxy appears relatively uniform, with a slight redder hue to the outer regions. The galaxy appears to be undergoing a low level of star formation activity. A low-level merger is a possible explanation of the shape and color distribution. 
