The galaxy presents as a moderately luminous object, exhibiting a somewhat smooth overall morphology, although with subtle underlying features suggesting potential past or ongoing disturbances. The color profile indicates a significant population of older stars, with a noticeable redder hue. There is a hint of a disk-like structure, but it is not prominently defined, suggesting a mixed morphological type or a galaxy undergoing a transition in structure. Faint tidal features or extended diffuse light could be present, requiring deeper observations for confirmation. The galaxy's shape appears generally rounded with some asymmetry. The limited color variation across the object implies relatively uniform stellar populations and a lack of significant current star formation. This galaxy may be in a later stage of its evolution, potentially having experienced a past merger event which has since settled into a smoother structure.
