The galaxy presents a generally smooth morphology, with a near absence of discernible spiral arm structures. The light distribution appears concentrated toward the center, indicating a prominent bulge. The overall shape is mildly elongated, exhibiting a slight deviation from a perfectly circular form. Color gradients suggest a radial change in stellar populations, with a bluer hue in the outer regions, possibly due to younger stars, and a whiter, more luminous core. There is no obvious signs of any ongoing major merger activity. The overall color suggests relatively low level of recent star formation, consistent with a mature stellar population. 
