The galaxy appears to be an elliptical galaxy with a smooth, diffuse light distribution. There is a noticeable central concentration of light, suggesting a bright nucleus or bulge. The overall shape is moderately elongated, exhibiting an aspect ratio of roughly 0.7, indicating it is not perfectly spherical. The galaxy presents a shallow Sersic profile, hinting at a possible compact dwarf elliptical form. The color gradient suggests a slightly bluer outer region compared to the central area. The lack of any distinct spiral arms or dust lanes supports its classification as an elliptical galaxy. Based on the red shift, the galaxy is relatively distant. There are no clear signs of any major ongoing mergers or tidal disturbances, although subtle features may be present at deeper image scales.
