The galaxy presents as an elongated, cigar-shaped object with a smooth, diffuse appearance. The central region exhibits a yellowish hue, suggesting a population of older stars. Progressing outward from the core, the color transitions to a bluer tone, possibly indicating younger stellar populations or ongoing star formation in the galactic disk. No distinct spiral arms or other prominent features such as dust lanes are immediately apparent. There are no signs of any major merger events, but a minor disturbance to the galaxy's structure is plausible.
