The galaxy presents as a moderately inclined spiral, possibly an Sa or Sb type, at a redshift of approximately 0.12. It exhibits a prominent, bright central bulge with a yellowish hue, indicative of an older stellar population. The disk appears somewhat flocculent with loosely wound spiral arms. Star formation seems present but not exceptionally vigorous, inferred from the subtle bluish regions within the spiral arms. There is a hint of minor disturbance or asymmetry in the outer regions of the disk, potentially due to a past minor merger event or tidal interaction. Overall, the galaxy displays a stellar mass comparable to that of the Milky Way.
