The galaxy presents a generally smooth, elliptical morphology, exhibiting a high degree of roundness. It appears relatively undisturbed, with no obvious signs of major mergers or significant tidal disruptions. Subtle features may be present, however, the image quality limits detailed morphological classification of any disk-like or irregular components. The galaxy displays a color profile suggestive of a population of older stars, leaning toward the redder end of the spectrum. This coloration indicates a relatively low ongoing star formation rate. Based on observed characteristics, this galaxy is likely a massive system.
