The galaxy appears as a generally smooth, centrally concentrated object with a somewhat rounded morphology. A slight elongation is visible, though the axial ratio suggests it is closer to spherical than highly flattened. The light distribution is smooth and shows a high degree of central concentration. It displays a color gradient, trending from a yellowish-white core to a slightly redder halo. There is little evidence of spiral arms or prominent dust lanes. No significant tidal features or indications of a major merger event are immediately apparent, although some minor asymmetry is present.
