The object appears to be a galaxy exhibiting characteristics suggesting a possible interaction or merger event. Its morphology is complex. The central region presents a smooth, concentrated light distribution that seems to dominate the structure. Extensions, potentially tidal features, are evident emanating from the central body. One such extension stretches away from the core, appearing more diffuse and elongated than the central condensation.

The color gradients observed suggest varying stellar populations. The core exhibits a reddish-orange hue, indicative of older stellar populations. The extended features, and to some extent the periphery of the central region, show hints of bluer coloration, which might indicate younger stars or ongoing star formation activity.

The overall structure suggests that this may be an intermediate mass system. This galaxy may not be fully relaxed, possibly undergoing a merger or gravitational disturbance. High-resolution imaging and spectroscopy are necessary to properly determine the dynamics of this galaxy, the nature of the observed features, and to accurately assess its stage of evolution.
