The galaxy appears as a central, concentrated light source. It has a roughly elliptical profile, though its shape is not perfectly symmetrical. I can discern a subtle extension of the galaxy's light beyond the core, implying a more extended structure. Its central region is comparatively bright and condensed, suggesting a high concentration of stars. There may be some minor disturbance in the galaxy's overall form, indicated by the slight asymmetry. The overall color suggests a moderate redshift, with a slightly redder tint relative to a bluer, younger galaxy. This may indicate an older stellar population. There is also the presence of some merger activity, though it is difficult to ascertain whether this is an ongoing major event.
