The galaxy appears as a relatively smooth, centrally concentrated object. The light distribution suggests a dominant spheroidal component, possibly an elliptical galaxy or a lenticular galaxy seen face-on. There is a slight elongation in its shape; however, it is closer to being round than a flattened disk. A yellow central region fades into a reddish halo. There does not seem to be any spiral arm structure visible. The color gradient, with a redder halo and yellower center, indicates potential differences in stellar populations. Given the smooth morphology and color, it is plausible that star formation is suppressed with a more dominant population of older stars. There is a very faint red object visible near the edge of the galaxy; it is impossible to tell whether this is related to the galaxy or not.
