The galaxy presents a generally smooth, elliptical morphology. Its color profile indicates a concentration of older stellar populations, appearing more yellow and red-toned in the central region. There is a subtle color gradient, with the core being slightly more yellow than the surrounding halo. The isophotes appear relatively regular, without significant distortions or tidal features, suggesting minimal recent interaction or merging events. The galaxy lacks any distinct spiral arm structure or prominent dust lanes. It appears to be a quiescent galaxy with a relatively low star formation rate, based on its color and morphology. The galaxy has a small angular size, and is likely at a non-negligible redshift.
