The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The color profile indicates a bulge dominated system with a notable absence of prominent spiral arm structures. The galaxy displays a significant red-shift, suggesting it is at a considerable cosmological distance. The relatively homogenous color distribution implies an older stellar population with reduced ongoing star formation within the galaxy. There is little evidence of recent or ongoing mergers, tidal disturbances, or significant dust lanes obscuring the galactic nucleus. The morphology is consistent with an early-type galaxy undergoing passive evolution.
