The galaxy presents as a somewhat elliptical structure with a noticeable central bulge. Its disk appears moderately inclined to our line of sight. The core exhibits a bright, concentrated luminosity suggesting a higher density of stars or potentially an active galactic nucleus. The outer regions of the galaxy appear fainter with smoother light distribution. The color profile seems to shift from yellowish-white in the central region to a slightly bluer hue towards the outer edges, suggesting the presence of younger, hotter stars in the galactic arms, though the colors are generally subdued. There is little apparent dust or distinct spiral arm structure visible in this image. The overall shape seems relatively smooth and undisturbed.
