The galaxy presents a generally smooth, elliptical morphology. It appears centrally concentrated, with a yellowish-white hue, suggesting an older stellar population dominates the light output. There is a subtle colour gradient, becoming slightly redder towards the center. There are minor irregularities in the galaxy's shape. The galaxy exhibits a slight asymmetry, hinting at possible gravitational interaction or recent accretion events. No distinct spiral arm structures are visible, furthering the assessment that the galaxy is primarily an elliptical type. The general lack of blue coloration would indicate that the galaxy is not currently undergoing significant star formation. The galaxy appears quite compact for a galaxy of its mass, implying a relatively high density of stars.
