The galaxy presents as a relatively smooth, elliptical-shaped object with a high degree of central concentration. The light profile appears well-defined, exhibiting a centrally-peaked distribution. There is a slight asymmetry observed in the galaxy's outer isophotes, suggesting a mild disturbance or interaction. The galaxy displays a color gradient, becoming redder towards the center, potentially indicating an older stellar population dominating the core. There is no significant evidence of spiral arms or prominent dust lanes within the galaxy's structure. The major axis of the elliptical shape is oriented at a position angle approximately 120 degrees counterclockwise from vertical. Overall, this galaxy is categorized as a massive galaxy with little current star formation.
