This galaxy exhibits a generally smooth, elliptical morphology with a concentrated central bulge. The light distribution appears relatively uniform, lacking distinct spiral arm structures or prominent dust lanes. The galaxy appears nearly circular in projection, suggesting it is either intrinsically spherical or viewed close to face-on. There is a slight color gradient, with the central regions appearing yellower compared to the bluer outer regions. This suggests a higher concentration of older stellar populations towards the center and a more recent episode of star formation in the outer regions. Given the smooth features with what appears to be some recent star formation, this could be an early-type spiral galaxy that has exhausted most of its gas supply, or a lenticular galaxy. There are also no obvious signs of major disturbances or ongoing merger events, though minor disturbances cannot be ruled out.
