The galaxy appears to be an interacting system, possibly in the early stages of a merger. The primary component shows a relatively smooth, centrally concentrated bulge with a faint, diffuse halo extending outwards. There is a secondary component appearing as a distinct knot or irregular feature located near the primary body. A tidal tail-like structure emanates, suggesting gravitational interaction. The primary bulge exhibits a slightly elongated morphology, with an apparent flattening. Color gradients within the galaxy are visible, with bluer colors more prominent in the halo regions and a yellower, redder hue concentrated in the central bulge, suggesting a possible difference in stellar populations. A significant portion of the image seems to be impacted by image artifacts.
