The galaxy presents as an elongated, cigar-shaped structure with a smooth, diffuse appearance. A distinct central bulge is not readily apparent, suggesting a relatively uniform distribution of stellar density across its length. The color profile indicates a dominance of older stellar populations, with a reddish-yellow hue concentrated primarily in the central regions, and a cooler bluish periphery. Faint indications of spiral arms or substructures are not discernible, and there is a lack of any significant dust lanes or patchy star formation regions. The overall morphology implies a galaxy that is either an elliptical nearing the spiral arm shape, or a very tightly wound spiral galaxy viewed at a high inclination angle. The lack of any obvious distortions in shape suggests no recent major merger events, however minor interaction may have occurred based on very slight asymmetry in the outer regions.
