The galaxy presents as an elongated, likely spiral or lenticular type, viewed at a significant angle, nearing edge-on. The central bulge appears prominent and shows a yellowish-orange hue, suggestive of an older stellar population. Faint extensions of light emanate from the central region, indicating the presence of a disk structure. These extensions appear relatively smooth, showing low star formation. A slight bluer tint is visible along the faint outer edges of the disk. There is no evidence of a major ongoing merger, however, there appears to be some form of minor distortion in the disk, and the overall shape of the galaxy is cigar shaped. Overall this seems to be a massive galaxy with a low rate of star formation.
