The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions into a diffuse halo. The core appears to be yellowish, indicative of an older stellar population dominating this region. The surrounding halo shows faint bluish tinges, suggesting the presence of some younger, hotter stars within the galaxy, or it might be an artifact of the image's processing. The overall form suggests a relaxed system, largely undisturbed, with no signs of prominent spiral arms or tidal features. The light distribution diminishes gradually from the core outwards.
