The galaxy presents as a roughly elliptical, relatively smooth, and concentrated light distribution. There is a bright central region, suggesting a prominent galactic nucleus. The color appears yellowish-orange in the center, transitioning to a bluer hue towards the outer edges. This may indicate the presence of an older stellar population in the core with younger, bluer stars in the surrounding regions, or perhaps a difference in dust content affecting the observed colors. No distinct spiral arms or other detailed features are readily apparent. There may be a very slight asymmetry to the galaxy’s overall shape, but it appears largely undisturbed.
