The galaxy presents an overall elliptical morphology, appearing largely smooth and centrally concentrated. Its core exhibits a yellowish-orange hue, suggestive of an older stellar population dominating the central region. Moving outward from the core, the color shifts to a slightly bluer tone, potentially indicating the presence of younger stars within the galaxy's disk or halo. There's a hint of a disturbed structure, possibly indicating an ongoing or recent minor interaction with another galaxy. No prominent spiral arms or bar features are discernible, supporting the smooth, elliptical classification. The galaxy appears relatively isolated within its immediate vicinity.
