The galaxy exhibits a somewhat elliptical morphology, with an apparent flattening. It presents a bright, concentrated central bulge that gradually fades into a less luminous disk. There is a notable color gradient, with the core appearing more yellow/white and the outer regions appearing bluer. This suggests an older stellar population concentrated in the center and younger stars forming in the outer regions. There is no clear evidence of spiral arms. It appears that there is minor disturbance to the shape, but generally nothing indicative of major interaction with another galaxy. The galaxy appears to be in a relatively quiescent state.
