The galaxy appears to be a relatively smooth, elongated system, viewed at a significant angle. Its shape is noticeably cigar-shaped, with the longest axis considerably greater than the shortest. The central region exhibits a reddish hue, likely indicative of an older stellar population. Moving outward from the center, the galaxy transitions to a bluer color. This suggests the presence of younger stars within the galaxy's disk. No distinct spiral arm structures are discernible. The overall smooth appearance, along with the color gradient, hints at a possible lenticular morphology. There are no obvious signs of major disturbances or mergers.
