The galaxy presents as an elongated, cigar-shaped structure. There appears to be a smooth, concentrated central bulge exhibiting a yellowish hue, possibly indicating an older stellar population. Surrounding the bulge, a fainter, bluish disk is observed, suggesting the presence of younger stars and ongoing star formation. The disk appears relatively smooth, with no obvious spiral arm structure visible in this image. There is a slight distortion or minor disturbance in the galaxy's morphology. Overall, the galaxy appears to be a relatively massive system with a moderate rate of star formation.
