The galaxy presents a largely smooth, elliptical morphology. The core exhibits a high surface brightness, appearing as a concentrated, almost stellar-like nucleus. The isophotes are generally round, with a minor elongation discernible in one direction. A subtle color gradient is observed, transitioning from a bluer hue in the central regions to a slightly redder tint in the outer halo. No obvious spiral arms or dust lanes are detected, indicating a relatively quiescent system. There may be some minor disturbances to the galaxy's structure, though they are not significant enough to suggest an ongoing major merger.
