The galaxy presents as a somewhat diffuse elliptical with a fairly smooth overall structure. The light is concentrated towards the center, which has a warm, yellowish hue. Moving outward from the core, the light gradually fades, with no clear signs of spiral arms or significant dust lanes. There are subtle variations in color across the galaxy, but the dominant color profile is on the redder end of the spectrum. The overall morphology suggests a galaxy with a considerable stellar mass but a low current rate of star formation. Its appearance is more akin to that of a mature galaxy, which may be undergoing a transition towards a more passive state in terms of star formation activity. There are no obvious signs of a major ongoing merger event, although minor disturbances cannot be ruled out. The light distribution appears to be consistent with a galaxy that is close to being symmetrical with a moderately elliptical shape.
