The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical, exhibiting a high degree of circularity in its overall shape. There is little discernible substructure, such as spiral arms or prominent dust lanes. The color profile is dominated by warmer hues, suggesting an older stellar population with relatively suppressed star formation activity. The galaxy appears to be isolated with no signs of interaction with other galaxies or major disturbances. The absence of strong blue colors indicates a low rate of on-going star formation.
