The galaxy presents as a centrally concentrated, smooth object. The light distribution is dominated by a bright, nearly circular core that fades gradually into the surrounding galactic halo. The core appears to be composed of an unresolved stellar population, contributing primarily to the G, R, and Z bands. There is a subtle color gradient visible, transitioning from a bluer hue in the center to redder tones further out from the nucleus. This suggests either a gradient in stellar populations, dust obscuration, or a combination of both. The galaxy lacks any readily apparent spiral arm structures, distinct dust lanes, or other features indicative of ongoing major star formation. There are no signs of any substantial tidal disturbances or evidence of a recent major merger event. Based on its morphology, this appears to be an elliptical galaxy or potentially a lenticular galaxy viewed nearly face-on.
