The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The light distribution is centrally concentrated, with a gradual fall-off in intensity towards the outer regions. The color appears relatively uniform across the galaxy, with a slight bluer hue towards the outer edges and a more yellowish color towards the center. This color gradient may indicate different stellar populations, with older, redder stars dominating the central regions, and younger, bluer stars present in the outer regions. There is no evidence of distinct spiral arms or a prominent disk structure. The galaxy shows no signs of recent or ongoing mergers or interactions, its overall structure appears undisturbed and relaxed.
