The galaxy presents a generally smooth morphology, with a somewhat elongated, cigar-shaped appearance. The central region exhibits a higher surface brightness, suggesting a concentrated nucleus. The galaxy displays a gradual decrease in luminosity towards its outer regions, with no apparent distinct spiral arm structures. Overall, the galaxy's color profile appears relatively uniform, with subtle color variations, possibly indicating differences in stellar populations across the galaxy. There is faint suggestion of a minor disturbance in the galaxy's overall structure, possibly due to tidal interactions with nearby galaxies. There appears to be a low rate of ongoing star formation within the galaxy.
