The galaxy presents a generally smooth, elliptical morphology with a bright, concentrated central bulge. The galaxy exhibits a blue-ish hue in its outer regions, which may indicate some ongoing star formation, albeit at a relatively low rate, or the presence of a younger stellar population compared to the core. The galaxy appears somewhat rounded, with no discernible spiral arms or distinct disk-like structure visible. There are hints of minor disturbances in the galaxy's morphology, but it does not appear to be undergoing a major merger event. The overall light distribution suggests a relatively evolved system.
