The galaxy appears as a centrally concentrated, elliptical structure. It exhibits a smooth, largely featureless morphology with a radial color gradient, transitioning from a yellowish core to a greenish outer halo. The galaxy's isophotes are generally round but are slightly elongated, presenting a mild ellipticity. There is no strong evidence of spiral arms or prominent dust lanes. The overall visual impression suggests a galaxy dominated by an older stellar population, with relatively little ongoing star formation in the central and halo regions. Some disturbances are detected but the structure is intact suggesting a lack of interaction or merging with other galaxies.
