This galaxy presents as a disk galaxy, likely viewed close to edge-on. A prominent bulge is observed with a yellowish hue. The disk appears flattened and relatively thin, displaying subtle color variations indicative of possible stellar populations or dust lane structures. The central bulge region dominates the overall luminosity. The disk extends further from the center and seems to have more blue stars on average compared to the center. There are indications of minor disturbance or asymmetry in the outer regions of the disk, potentially suggesting tidal interactions or recent minor merger events. The disk overall, is relatively smooth. No obvious spiral arm structure is discerned in this image. The galaxy appears actively forming new stars at a moderate rate. Overall this galaxy is fairly massive, and its specific star formation rate suggests it may be entering a transitional stage in its evolutionary history.
