This galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a high degree of central concentration with a gradual decrease in luminosity outwards. The color profile indicates a dominant population of older stars, with a yellowish-white hue suggesting low ongoing star formation. There is little evidence of spiral arms or distinct features, implying it is likely an early-type galaxy, possibly an elliptical or lenticular galaxy. The shape is somewhat elongated, but not extremely so, resembling an oval with a possible slight flattening. There appears to be no obvious signs of a major merger, although minor distortions or disturbances cannot be ruled out from this image alone.
