The galaxy presents as a concentrated, elliptical morphology. It exhibits a smooth, relatively featureless structure lacking defined spiral arms or a prominent dust lane. The color profile suggests a population of older stars, indicated by the yellowish-orange hue dominating the central region. The galaxy appears moderately luminous, with a diffuse halo extending beyond the central core. There is no discernible evidence of ongoing major merging activity or significant tidal disturbances. Based on its general form and color characteristics, this galaxy likely has a high degree of internal order and stability.
