The galaxy presents as a relatively small, elliptical structure. Its overall light distribution appears smooth and centrally concentrated, with a high degree of roundness. There's a lack of discernible spiral arms or a prominent disk. The galaxy's core exhibits a brighter, more intensely luminous region, which fades gradually towards the edges. No significant dust lanes or patches are visible. The color profile suggests a population of older stars, giving it a yellowish hue. There is no evidence of recent or ongoing major mergers or tidal disturbances. The galaxy is likely undergoing a low rate of star formation.
