The galaxy presents as a somewhat diffuse, elliptical-like structure with a concentrated, bright central bulge. The core region exhibits a yellow-orange hue, suggesting a population of older stars. There is a subtle color gradient moving outwards from the center, with the outer regions appearing slightly redder. No distinct spiral arms or bar features are discernible within the resolution limits of the image. There appear to be some hints of tidal disturbances or faint features suggesting a possible past minor merger event. The galaxy is overall relatively smooth.
