The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a generally smooth morphology. It presents an elongated, cigar-like shape, suggesting a disk-like structure viewed at a significant inclination angle. A bright, concentrated central bulge is evident, appearing yellowish-white, possibly indicating an older stellar population within the nucleus. The outer regions of the galaxy show a fainter, bluer hue, suggesting the presence of some younger, star-forming regions. No prominent spiral arms are discernible from the image, hinting that either any spiral structure is tightly wound or that star formation is relatively subdued compared to later-type spiral galaxies. There is no obvious visual evidence of any major merger events or significant tidal disturbances in its immediate vicinity. The overall structure seems relatively undisturbed.
