The observed galaxy appears to be a relatively compact object, exhibiting a somewhat elliptical morphology. A bright, concentrated central region dominates its structure, suggesting a high stellar density in the core. Surrounding this central region is a more diffuse, extended halo. There is a subtle disk like structure with hints of spiral arms or extended structures surrounding the central bulge. The overall color distribution indicates variations in stellar populations, with bluer hues evident in the outer regions, possibly indicating younger stellar populations. Some irregularities or distortions are visible in the galaxy's shape, suggesting a possible gravitational interaction or recent merger event. Overall, this galaxy displays characteristics of a galaxy with signs of potential dynamical disturbance.
