The galaxy presents as an elliptical structure, exhibiting a smooth, concentrated morphology. The central bulge appears bright and yellowish, potentially indicative of an older stellar population. A faint, extended halo surrounds the core, appearing more greenish in hue, perhaps suggesting the presence of younger stars or ionized gas. There is no apparent spiral arm structure, bar, or significant dust lane obscuration visible in this imagery, which supports the identification of an elliptical galaxy. The overall color profile implies a galaxy with a moderate redshift, based on the apparent brightness and the subtle color shifts. There is no evidence of any major interaction or merging events affecting this galaxy. There may be some minor disturbances, but the overall structure of the galaxy has a singular distinct form.
