The galaxy presents as a luminous, centrally concentrated object, exhibiting a generally smooth morphology. A significant fraction of its light appears to originate from a spheroidal component. The galaxy displays a yellow-red hue. This central spheroidal component has an apparent moderate ellipticity. Further away from the galactic center, we can see what seems to be a galactic disc that is showing some features and a blue hue, suggesting some degree of ongoing star formation. There appears to be no significant presence of tidal tails or other indicators of ongoing major merger activity, although a minor disturbance cannot be ruled out based on the image alone. The object overall appears to be well-defined with no signs of being an artifact.
