The galaxy presents as a largely smooth, elliptical morphology. The light distribution is concentrated towards the center, with a noticeable radial decrease in surface brightness. A yellowish hue dominates the central region, suggestive of an older stellar population. Surrounding the core, there is a subtle presence of bluer light, perhaps indicating the presence of some younger stars, albeit in smaller quantities compared to the older population. The overall shape is elliptical with a high degree of roundness. There is no obvious evidence of spiral arms or a prominent disk. There are no signs of a major ongoing merger or significant tidal disturbances. The galaxy appears relatively undisturbed.
