The galaxy presents as a centrally concentrated, luminous object with a smooth, elliptical morphology. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. The outer regions display a gradual fading and reddening in color. This color gradient likely indicates a decrease in stellar age or an increase in dust extinction with increasing distance from the galactic center. There appears to be minimal evidence of spiral arm structure or active star-forming regions within the observed area. A very faint reddish source is visible at the lower edge of the galaxy. The overall appearance is indicative of an evolved system with a high degree of sphericity.
