The galaxy appears to be a spiral galaxy, possibly of the Sa or Sb type, viewed at an oblique angle. The central bulge appears prominent and concentrated, exhibiting a yellow-white hue, suggesting an older stellar population. Faint spiral arms extend from the central bulge, displaying a bluer color, indicative of ongoing star formation. These arms are not well-defined and appear somewhat flocculent. There is evidence of dust lanes within the spiral arms. A possible tidal tail or distorted structure is visible to one side, potentially indicating an interaction or merger event in its recent history. Overall, the galaxy exhibits a moderate degree of star formation, with signs of both old and young stellar populations. The shape is mostly rounded. There seems to be minor disturbance due to the possible merger or interaction.