The galaxy presents as a largely featureless, elliptical morphology. Its color profile suggests an older stellar population, exhibiting a yellowish-red hue indicative of evolved stars. The light distribution appears smooth and centrally concentrated, with a gradual decrease in luminosity outwards from the core. There is no evident disk structure or spiral arm formation. No significant tidal features or signs of recent major mergers are apparent. Minor irregularities in the outer regions could potentially indicate minor disturbances or past interactions. The object's generally homogenous appearance indicates a well-mixed stellar population, typical of elliptical galaxies. The relatively high smoothness fraction supports this assessment.
