The galaxy presents as a centrally concentrated, elliptical-like structure. It appears generally smooth with no clear spiral arms or bar features. The light distribution suggests a dominance of an older stellar population. There is a subtle color gradient, with the central region exhibiting a slightly bluer hue compared to the outer regions. The galaxy's shape is close to round, although not perfectly circular. There appears to be a very minor disturbance in the shape of the galaxy, but it is largely an isolated system.
