The galaxy presents as a highly elongated, cigar-shaped morphology. Its central region exhibits a concentrated luminosity, appearing relatively smooth in texture. The outer regions of the galaxy, or disk, show a gradual decrease in surface brightness with indistinct boundaries, appearing diffuse. There is evidence of some asymmetry or minor disturbance in the galactic structure. The overall color profile suggests a population of older stars, primarily a yellowish hue, with limited evidence of ongoing or recent star formation. The galaxy is significantly inclined relative to our line of sight.
