The galaxy appears to be a flattened, disk-like system oriented at a significant angle relative to our line of sight. The central bulge is relatively prominent and exhibits a yellowish-orange hue, suggesting a population of older stars. Moving outward from the bulge, the color transitions to a slightly bluer shade, potentially indicating the presence of younger stars and regions of active star formation, although these features are not highly pronounced. The overall shape is elliptical, with an estimated ratio of the minor to major axis suggesting a highly inclined disc. The galaxy appears relatively smooth and lacks distinct spiral arm structures, which might indicate a later-type spiral galaxy, or a lenticular galaxy. There is no obvious signs of interaction, such as tidal tails or distorted morphology. Overall, the galaxy seems like a stable, well-defined system at a considerable distance.
