The galaxy presents as a centrally concentrated object with a smooth, diffuse appearance, suggestive of an elliptical morphology. The central region exhibits a bright, relatively well-defined core, indicating a high stellar density. Moving outwards, the light gradually fades, transitioning into a fainter, more extended halo. There is a subtle color gradient from the center outwards. The central core is slightly yellowish-white, while the outer regions appear more bluish. This may indicate a difference in stellar populations, with older, redder stars dominating the core and younger, bluer stars contributing to the outer halo. I don't note any pronounced spiral arms or dust lanes, and there are no apparent signs of recent major merger activity in the galaxy's morphology, such as tidal tails or distorted shapes.
