The galaxy appears to be a spiral galaxy, viewed at a slight angle relative to face-on. The central bulge is prominent and exhibits a yellowish hue, potentially indicating an older stellar population. Faint spiral arms emanate from the bulge, displaying a somewhat flocculent structure. These arms have a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation. There is evidence of dust lanes within the spiral arms, which contribute to the patchy appearance. Overall, the galaxy has a fairly regular morphology without significant signs of tidal disturbances or major mergers.
