The galaxy appears as a diffuse, centrally concentrated object with a subtle, almost imperceptible disc-like structure. Its color profile suggests a population of predominantly older stars, exhibiting a reddish-yellow hue. There are hints of bluer regions in the central area, indicating ongoing or recent star formation, although it appears relatively low. Some distortion is visible in the surrounding area, possibly showing signs of an ongoing or recent merger event with another galaxy, or a minor tidal interaction. The galaxy lacks any prominent spiral arm structures or a bright, active galactic nucleus; it is comparatively faint, and not extremely active.
