The galaxy appears as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a noticeable lack of spiral arm features, lending to its overall elliptical classification. The color profile suggests an older stellar population, with a yellowish hue dominating the central region. The galaxy displays a high degree of circularity. There is no evidence of a recent major merger, or significant tidal disturbances. Star formation appears low, likely due to the more evolved stellar population.
