The galaxy presents as a disk-dominated system, viewed at a significant angle. The central region exhibits a concentrated bulge. Overall, the galaxy appears relatively smooth with some indications of spiral arm structure. There is a slight color gradient, with a redder core and bluer disk, likely indicating the presence of older stellar populations in the core and ongoing star formation in the arms. There is no clear evidence of tidal disturbances or interaction with other galaxies in this image.
