The galaxy presents as a smooth, elliptical structure. Its light profile is centrally concentrated, with a gradual decrease in intensity towards the outer edges. The core exhibits a yellowish-orange hue, indicative of an older stellar population. There is a slight flattening of the galaxy, giving it a cigar-like appearance, suggesting it may be an elliptical galaxy viewed at an angle. No distinct spiral arms or prominent dust lanes are visible. There are no obvious signs of ongoing major mergers or tidal disturbances in this image.
