The galaxy presents as a relatively smooth, elliptical-like structure. It appears centrally concentrated with a bright, yellowish core, potentially indicative of an older stellar population. The outer regions exhibit a gradual fading in luminosity and a slightly redder hue, suggesting a possible decrease in star formation activity towards the galaxy's periphery. There is little evidence of distinct spiral arms or significant dust lanes, aligning with the likely classification as an elliptical or lenticular galaxy. Based on the smoothness and lack of major disturbances, it does not appear to be undergoing a major merging event, although minor tidal features are not ruled out given the image resolution. The overall shape is generally round, with a hint of elongation. The galaxy's color indices indicate it has undergone a considerable redshift.
