The galaxy presents as a spindle-shaped structure, strongly suggesting a highly elongated or cigar-shaped morphology. The central region appears brighter and exhibits a yellowish-white hue, possibly indicative of an older stellar population. Fainter, bluish arms or extensions emanate from the central bulge, suggesting the presence of younger, hotter stars and potential star-forming regions, though these features are not sharply defined. There are slight irregularities or disturbances in the outer regions of the galaxy. The overall impression is that of a galaxy at a considerable distance.
