The galaxy appears to be an elliptical galaxy, exhibiting a smooth, symmetrical structure with no readily discernible spiral arms or prominent dust lanes. The core of the galaxy is noticeably brighter and more concentrated, indicating a higher density of stars. The galaxy exhibits a subtle color gradient, with the central region appearing slightly more yellow/red in hue, possibly indicating an older stellar population compared to the outer regions which appear bluer. The overall shape is somewhat elongated, presenting an intermediate ellipticity; not perfectly spherical, but not excessively flattened either. There is little evidence of ongoing major merger activity, although some minor disturbances may be present given the fuzziness of the outer edges, and some activity in star formation.