The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a bright, concentrated luminosity, suggesting a dense population of stars. The color of this central bulge appears yellowish-white, possibly indicating an older stellar population.

Moving outward from the core, the luminosity gradually decreases. Fainter, bluish hues are visible at the edges of the disk, hinting at ongoing star formation activity within spiral arms. No distinct, well-defined spiral arms are apparent. This could be due to the viewing angle, dust obscuration, or a smoother distribution of star formation.

The overall structure suggests a spiral galaxy, likely of a later type, or possibly a lenticular galaxy. There is no visual evidence of any major mergers or significant tidal distortions in the immediate vicinity. The galaxy appears relatively undisturbed, maintaining a somewhat smooth and regular morphology. 
