This galaxy appears to be a relatively face-on spiral galaxy. The central bulge is prominent and exhibits a yellowish hue, suggestive of an older stellar population. The disk of the galaxy is tilted slightly relative to our line of sight, giving it an elongated, cigar-like appearance. A hint of bluer light is visible within the disk, indicating the presence of some younger stars. No obvious spiral arm structure is apparent, possibly obscured by dust or low star formation activity. The galaxy exhibits some disturbance, hinting at a possible past interaction with another galaxy, though no merging is currently visible. The galaxy is moderately sized, suggesting a significant stellar mass. Based on the color and morphology, the star formation rate appears to be suppressed. 
