The galaxy presents a roughly elliptical morphology, although the edges are irregular and somewhat undefined. The central region exhibits a high surface brightness, appearing almost uniformly bright white with a slight blue hue, suggestive of a substantial population of young, hot stars or a luminous active galactic nucleus. Moving outward from the center, the galaxy transitions through shades of cyan and then darker blue, implying variations in stellar population or dust content, which may be causing differential absorption of light. A faint, diffuse reddish tinge can be seen near the outer perimeter. The lack of clear spiral arm structure, combined with the smooth appearance, suggests this may be an elliptical or lenticular galaxy. There may be evidence of a slight merger or tidal disturbance occurring, though the evidence is weak based on this image alone.
