The galaxy presents as a somewhat disturbed system, exhibiting a non-smooth morphology suggestive of a possible interaction or ongoing merger. The central region displays a condensed, bright core with a pale yellow hue. Extending outward from the core, the disk shows patchy, irregular features and spiral arm segments with bluer components, which could point to younger stellar populations and active star formation. Fainter, diffuse emission surrounds the main body, possibly indicating tidal debris or extended stellar halos resulting from gravitational disturbances. The overall color index suggests a galaxy that is not purely quiescent but exhibits signs of recent or current star formation activity. There are components of both a smooth shape, and more featured disturbances, possibly suggesting some sort of ongoing galactic interaction.
