The galaxy presents as a centrally concentrated elliptical system, appearing smooth in texture with no discernible spiral arm structure or dust lanes. The core region exhibits a bright, diffuse glow, indicative of a high stellar density. Moving outward from the core, the light intensity gradually decreases, suggesting a spheroidal distribution of stars. The outer edges appear slightly elongated, moving from the upper left to the lower right, though the overall shape remains largely ellipsoidal and well-defined. There are no visible signs of recent major merger events or significant tidal distortions within this observed field. The galaxy's color is predominantly yellowish-orange, indicative of an older stellar population with fewer hot, young, blue stars, and a low rate of star formation.
