The galaxy presents as a centrally concentrated object, roughly circular in projection. The light distribution appears smooth, with no obvious spiral arm structures or distinct features visible. There is a gradual decrease in light intensity from the center outwards, suggesting a bulge-dominated morphology. The color profile indicates a dominant yellow/orange hue, which could indicate an older stellar population with minimal ongoing star formation. The object exhibits a high degree of symmetry, indicating it is likely undisturbed or in a relatively stable state. There is a slight ellipticity; it is not perfectly circular. Its measured size is moderate. 
