The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct disk structure. The light distribution is concentrated towards the center, gradually decreasing in intensity outwards. There is a slight elongation, suggesting it is not perfectly spherical, but rather somewhat spheroidal in shape. Its color indices indicate a population of older stars, giving it a redder appearance. The galaxy is relatively isolated, showing no obvious signs of ongoing or recent major mergers, though subtle disturbances cannot be ruled out. It is moderately sized. The absence of bright, blue regions suggests a relatively low star formation rate.
