The galaxy exhibits a generally smooth morphology, appearing centrally concentrated with a diffuse outer halo. There is evidence of some internal structure, possibly a weak disk-like component or arm-like features, but these are not sharply defined. The color profile suggests a relatively evolved stellar population, with a central region appearing more red or yellow, indicative of older stars. There are some blue tinges toward the outer parts of the object. The object appears slightly elongated, without any extreme distortions or tidal tails to indicate a recent major merger event. The galaxy is likely a relatively massive system undergoing active, ongoing star formation.
