The galaxy appears as a slightly elongated, concentrated central bulge with a smooth, diffuse halo extending outwards. The color profile suggests a dominant population of older stars, exhibiting a yellowish-red hue throughout. The shape shows a moderate deviation from perfect circularity, leaning towards an elliptical morphology. There is no visible evidence of spiral arms or significant dust lanes. No tidal tails or other clear signs of recent major merger events are discernible, though subtle disturbances may be present in the outer halo. The galaxy appears relatively isolated.
