This galaxy exhibits a relatively smooth morphology, with a predominantly round shape. The central region displays a higher concentration of light, suggesting the presence of a substantial galactic nucleus. There is some indication of disturbance in the galaxy's overall structure, potentially resulting from a minor interaction or internal dynamics. The light distribution appears somewhat asymmetrical. A faint blueish halo surrounds the galaxy, possibly indicative of ongoing, though not particularly high, star formation within the galaxy. There appear to be two distinct bright regions, indicating that this is a possible merger. 
