This galaxy presents a distinct, elongated morphology, appearing cigar-shaped with a relatively smooth overall texture. A central bulge is visible, exhibiting a yellowish-orange hue suggesting an older stellar population. The galaxy fades in intensity from its core outwards, which appears to be composed of a disk with faint spiral arm features, possibly obscured by dust or viewed at a high inclination angle. The outer regions display a bluer tint, indicative of younger, hotter stars and ongoing star formation. There is no obvious evidence of strong tidal interactions or mergers based on this visual inspection. The galaxy appears largely undisturbed.
