The galaxy presents as a single, somewhat smooth, centrally concentrated object. Its overall morphology is relatively round. A significant fraction of the galaxy’s light appears to be emitted from what seems like a relatively compact core region. I notice a yellowing of light from one of the galactic core regions, and the appearance of a greener hue towards the edge of this area. Further examination is needed to understand the potential presence of merging phenomena, or minor disturbances within the galaxy, as the core appears to be split in two.
