This galaxy appears to be a spiral galaxy with a moderate bulge. There is evidence of loosely wound spiral arms exhibiting a patchy distribution of star formation. The spiral structure appears somewhat disorganized and disturbed suggesting a possible interaction or minor merger event with another galaxy. There is no clear presence of a bar. The galaxy exhibits a mixed population of stars, with evidence of both older, redder stars in the bulge and younger, bluer stars in the spiral arms, signifying ongoing star formation activity. The galaxy exhibits a disk oriented face-on relative to our line of sight.
