The galaxy exhibits a generally elliptical morphology, with a smooth appearance suggestive of a relatively evolved system. There is a clear central bulge, characterized by a yellowish-white hue, indicating a higher concentration of older stellar populations. The disk, viewed at a high inclination, appears flattened and somewhat elongated, lending a cigar-like shape to the galaxy. The color of the disk transitions from a yellow-white near the bulge to a bluer tint further from the center, implying the presence of younger, hotter stars in the outer regions. There is no clear evidence of spiral arm structure or significant dust lanes. A small amount of faint disturbance could be present.
