This galaxy presents as a roughly elliptical shape, elongated along its major axis. The central region exhibits a bright, concentrated nucleus. Proceeding outward, the luminosity gradually decreases, suggesting a smooth distribution of stars. The primary color of the galaxy is a yellowish-orange hue, which implies a population of older stars. We can see a faint hint of bluer hues at the edges of the disk, possibly indicating more recent star formation. There appears to be some slight irregularity in the structure suggesting the possibility of a minor gravitational disturbance event.
