This galaxy presents as a relatively smooth, disk-shaped structure. It exhibits a prominent central bulge, appearing more yellow or golden in color, suggesting an older stellar population concentrated in the core. The disk surrounding the bulge shows a bluer hue, indicating the presence of younger, hotter stars and possible ongoing star formation. The galaxy's shape is elongated, leaning towards a cigar-like shape. No strong evidence of spiral arms is immediately apparent in this image. The outer regions of the disk fade gradually into the background, lacking sharp boundaries. Overall, the galaxy seems to be relatively undisturbed, showing no signs of a recent major merger or strong tidal interactions, although minor disturbances or internal structures might be present upon closer inspection.
