The galaxy exhibits a generally smooth, elliptical morphology. Its core is relatively bright and concentrated, with a yellowish hue. The overall shape is largely round, appearing neither significantly flattened nor elongated. There is a noticeable color gradient, transitioning from a brighter, possibly younger, stellar population near the center to a more homogenous, reddish halo. No prominent spiral arms or dust lanes are discernible. There is no evidence of major mergers or significant tidal disturbances. The galaxy may have either completed star formation processes or is producing new stars at a slow rate, but it shows a lack of features associated with active starburst regions.
