The galaxy presents a generally smooth, elliptical morphology. There's a slightly elongated, somewhat flattened shape, appearing neither perfectly spherical nor highly elongated. The light distribution indicates a central bulge region, which has a more intense and concentrated brightness. The galaxy's color profile suggests a relatively old stellar population, exhibiting more light in the redder bands of the spectrum, though with a slight presence in the blue bands. The image shows no evidence of significant dust lanes, spiral arms, or other prominent features indicative of active star formation. There also appear to be no obvious signs of any major ongoing merger events or strong tidal disturbances. The galaxy's size appears relatively compact.
