The galaxy presents a smooth, elongated morphology, appearing cigar-shaped. Its light distribution indicates a relatively smooth profile, suggesting a lack of prominent spiral arms or significant star-forming regions. The object displays a color gradient, shifting from bluer tones at one end to redder hues towards the opposite end and center. This could indicate variations in stellar populations or dust content across the galaxy, with the bluer regions potentially hosting younger stars. The galaxy shows no obvious signs of major mergers or tidal disturbances but appears to have a minor disturbance. It is likely a disk galaxy but could possibly be an elliptical galaxy.
