This galaxy presents as a relatively smooth, centrally concentrated object. The overall shape is elliptical, displaying an intermediate axial ratio, appearing neither perfectly circular nor highly elongated. A slight color gradient is discernible, with the core region exhibiting a bluer hue compared to the outer regions, which tend towards redder colors. The galaxy does not show any obvious signs of ongoing major mergers, though there is a hint of minor disturbance in the form of faint extended light that may point to past gravitational interactions. The image suggests the galaxy is a moderately sized object with relatively low star formation activity, and the light is dominated by an older stellar population compared to what would be expected in a vigorously star-forming spiral galaxy.
