The galaxy presents as a relatively smooth and centrally concentrated object, exhibiting a largely elliptical morphology. It appears to be fairly compact, with a concentrated central bulge that gradually diffuses outward. The light profile suggests minimal discernible spiral arm structure or prominent disk features. The galaxy's color index indicates a redder, more evolved stellar population throughout the galaxy, this is especially pronounced in the center of the galaxy. There is no evidence of significant ongoing star formation activity based on the color and smoothness. No signs of any tidal disturbances or close companion galaxies are evident in this observation. This galaxy is likely a large elliptical galaxy.
