The galaxy presents as a luminous, centrally concentrated object. The core region is bright and appears nearly spheroidal, exhibiting a smooth morphology. The overall color profile suggests a population of older stars, with a slight bluer hue emanating from the central region. Faint hints of extended structure are visible, potentially indicating a disk-like component, or a disturbed morphology. Given the apparent smoothness and central concentration, this object may be an elliptical galaxy or a spiral galaxy with a dominant bulge. There appears to be some type of companion or feature with no obvious connection to the main body of the galaxy, but likely interacting with it.
