The galaxy presents a primarily smooth morphology, appearing as a single, relatively round object. There is a slight elongation, suggesting a minor deviation from perfect circularity. A color gradient is observed, with the central region appearing more yellow, potentially indicating a higher concentration of older stellar populations. The outer regions exhibit a subtle blue tint, which may point to the presence of younger, hotter stars, or ongoing star formation, though the rate appears to be relatively low. There may be a faint, disturbed region in the outer disk of the galaxy, possibly indicating minor gravitational interactions with another galaxy. Overall, the galaxy appears to be a massive system at a considerable distance, with a morphology that suggests it could be an elliptical or lenticular galaxy.
