The galaxy presents a generally smooth, elliptical morphology, with an apparent axis ratio indicating a moderate degree of flattening. The light distribution appears centrally concentrated, suggesting a dominant bulge component. There is a subtle color gradient from the central region outward. The core is a pale red/yellow hue, potentially indicating an older stellar population. Fainter blue-green light is present in the outer regions, possibly suggesting younger stars or ongoing star formation. No prominent spiral arms or other distinct features are readily apparent in this image. The galaxy exhibits slight asymmetry or a very subtle disturbance, which could indicate a past minor interaction or merger event, although the overall structure remains relatively undisturbed.
