The galaxy appears to be comprised of two distinct components. The first component is a centrally concentrated, yellowish-white, smooth, and relatively round structure. This component dominates the overall luminosity of the system.

The second component, located to the lower left of the first, exhibits a more elongated, diffuse morphology. It presents a bluer hue compared to the central structure, possibly indicative of younger stellar populations. There is a hint of a tidal tail or stream extending from the lower elongated component.

The system appears relatively undisturbed, although the presence of the elongated feature suggests possible past interactions or ongoing internal processes shaping the galaxy's structure.
