The galaxy presents as a smooth, elongated object with a distinct central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the core, the disk appears bluish, possibly indicative of more recent star formation activity. The galaxy's shape is noticeably cigar-shaped, lacking any prominent spiral arm structures or significant dust lanes in this image. There appears to be no signs of any major merging events or significant disturbances in the galaxy's overall structure. The morphology is consistent with that of an early-type spiral galaxy.