This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a high degree of central concentration, with the majority of its luminosity emanating from a bright, yellowish core. There is little evidence of distinct spiral arm structures or dust lanes. The overall shape is generally rounded, with only a slight deviation towards an elongated form. No major disturbances are visible, suggesting that the galaxy is not currently undergoing a major merger event, although there may be some slight indications of minor interactions or tidal features in the surrounding region. The galaxy presents as largely featureless beyond the gradual decrease in luminosity from the core to the outer edges. The color profile suggests a population of older stars, with a possible absence of significant recent star formation.
