The galaxy presents as a centrally concentrated, elliptical morphology. The galaxy's light profile appears smooth, with no visually discernible spiral arms or distinct features. The shape deviates slightly from perfect circularity, exhibiting a mild elongation, trending towards a cigar shape. There are no obvious signs of ongoing major merger activity. However, a minor asymmetry or disturbance cannot be ruled out, and the possibility of a past minor interaction is not ruled out. The galaxy displays a color gradient, transitioning from yellow in the core, to redder hues in the outer regions. The central region exhibits a brighter luminosity as compared to the outer edges.
