The galaxy presents a somewhat diffuse appearance, characterized by a central concentration of light that gradually fades outwards. The overall structure appears relatively smooth, suggesting a lack of prominent spiral arms or a well-defined disk. There might be some minor irregularities within the galaxy's structure, hinting at past interactions or internal dynamics. The galaxy seems to be more elongated than circular, possibly indicating an elliptical shape. The color distribution appears fairly uniform across the galaxy, with a subtle shift towards redder hues in some regions and bluer hues in other regions. This color variance could be related to differing stellar populations or the presence of dust lanes. The galaxy’s periphery lacks a sharp boundary, appearing to blend gradually into the background sky.
