The galaxy presents a generally smooth, elliptical morphology. Its color profile appears largely uniform across its visible extent, with a slight gradient from a brighter, central region to fainter outer edges. There appears to be no distinct spiral arm structure or noticeable dust lane obscuration. The overall shape is approximately circular, suggesting a low degree of inclination relative to the line of sight. The light appears to be concentrated in the center. There is no evidence of significant tidal disturbances or ongoing major merger events. The lack of strong color variations indicates a relatively quiescent star formation history, consistent with a predominantly older stellar population.