The galaxy exhibits an elongated, cigar-shaped morphology. It appears relatively smooth, with a concentrated central bulge that fades into a disk-like structure. The light distribution is not uniform; the central region is brighter and redder, indicative of an older stellar population. Moving outwards, there are hints of bluer colors, perhaps indicating younger stars. The galaxy shows a high degree of ellipticity. No distinct spiral arms or prominent dust lanes are discernible in this image, suggesting it might be an elliptical or lenticular galaxy. The overall structure appears undisturbed, with no major signs of ongoing mergers or tidal interactions.
