The galaxy presents as a singular object, exhibiting a somewhat smooth morphology. The central region displays a bright, concentrated luminosity, suggesting a significant stellar population density. The overall shape tends towards rounded, with only a slight deviation from perfect circularity. Subtle colour variations are observed, with the core appearing more yellow/orange in hue, possibly indicating an older stellar population and diminished star formation activity in the nucleus. Fainter, bluer extensions are marginally visible, suggestive of ongoing, although likely low, levels of star formation. There is a slight asymmetry in the brightness distribution indicating the possibility of a minor interaction or disturbance but no obvious signs of an ongoing merger. 
