The galaxy presents as a moderately bright, elliptical-like structure. Its core is luminous and appears yellowish-white, indicating a population of older stars. The galaxy lacks distinct spiral arms or a prominent disk. There is a hint of ellipticity, with the major axis oriented roughly northeast to southwest. A subtle color gradient is observed moving outwards from the core, transitioning to a more reddish hue in the outer regions, again suggesting an aging stellar population. The overall texture is smooth, showing no signs of significant dust lanes or active star-forming regions. The galaxy appears relatively isolated and undisturbed, maintaining a regular and symmetric morphology. The slight ellipticity suggests a degree of intrinsic angular momentum, even in the absence of a clear disk.
