The galaxy presents as an elongated, cigar-shaped structure. Its color profile suggests a central concentration of older stellar populations, exhibiting a yellowish hue. Progressing outwards from the galactic center, the color shifts toward bluer tones, potentially indicative of ongoing or recent star formation within the galaxy's disk. No distinct spiral arm structures are readily apparent, and there are no signs of major disturbances or ongoing mergers with other galactic bodies.
