The galaxy presents as a centrally concentrated object with a generally smooth appearance. The core exhibits a bright, yellowish-white hue, suggesting a high density of older stellar populations. A slightly flattened, elliptical morphology is observed. Faint, diffuse extensions emanate from the core region, displaying a bluer tint, which could indicate the presence of some ongoing star formation within the outer regions. There appears to be minor asymmetry in the faint extensions, potentially indicating a slight gravitational interaction or past merger event. The overall color profile leans towards the redder end of the spectrum, which is expected given the estimated redshift.
