The galaxy presents a relatively smooth, elliptical morphology with minimal discernible features. Its overall shape is predominantly round. There is no apparent disk structure or spiral arm morphology. The core region is bright and centrally concentrated, displaying a yellowish hue, indicative of an older stellar population. Surrounding the core, a broader, less intense halo extends outwards. This halo exhibits a bluish tint, potentially signifying the presence of younger, hotter stars or a contribution from ongoing star formation, although this appears to be at a low rate. The image reveals no signs of ongoing major mergers or significant tidal disturbances, suggesting the galaxy is relatively isolated and undisturbed.
