The galaxy presents an overall bluish hue, suggestive of ongoing star formation. The central region is noticeably brighter and more concentrated, with a yellowish-white appearance, potentially indicating an older stellar population and a higher density of stars. Fainter, irregular extensions are visible emanating from the main body of the galaxy, hinting at tidal interactions or recent merger events. The disk appears somewhat disturbed or amorphous, lacking well-defined spiral arms, though it is not uniform. There appears to be a possible companion galaxy interacting with the main galaxy.
