The galaxy presents as a spiral galaxy with a relatively face-on orientation. Faint spiral arms emanate from the central region. The arms appear somewhat flocculent and less defined, suggesting a possible lack of grand design structure. Dust lanes are subtly visible within the spiral arms, indicating ongoing star formation regions. The bulge is relatively small compared to the overall disk size, possibly a pseudo-bulge or a relatively young classical bulge. There appears to be little to no disturbance from any merger event. The blue color indicates a population of young, hot stars, suggesting current or recent star formation activity.
