The galaxy presents as a relatively smooth, centrally concentrated light distribution, appearing elliptical or lenticular in morphology. The radial color gradient suggests a population of older stars dominating the overall light, with some evidence for bluer, potentially younger stars in the outer regions. No prominent spiral arms or obvious dust lanes are apparent. The overall shape is fairly circular, lacking significant elongation or signs of tidal disruption that might indicate recent merger activity, although some minor disturbances cannot be ruled out based on this image alone. The galaxy is quite large and massive.
