The galaxy presents as a generally smooth, elliptical morphology. There is a slightly elongated structure, trending toward a rounded form. A concentration of light is observed toward the galactic center, with a gradual fading towards the outer edges. There are subtle variations in color across the galaxy, with the central region exhibiting a yellowish hue, suggesting an older stellar population. The periphery shows a slight hint of bluer tones, indicating the possibility of some younger stars, but overall, the stellar population appears relatively aged. There is no discernible spiral arm structure or evidence of significant dust lanes. Furthermore, there's a lack of any significant tidal disturbances or indications of recent merger activity within the image's resolution.
