The galaxy presents as an elongated, disk-shaped structure, oriented nearly edge-on from our vantage point. A prominent central bulge dominates the luminosity profile, exhibiting a smooth, spheroidal morphology. The bulge appears to be the brightest region of the galaxy. The disk component is subtle, appearing as a faint, diffuse extension along the major axis. No distinct spiral arms or prominent dust lanes are discernible. The overall color of the galaxy appears to be relatively uniform, with a slightly bluer hue concentrated towards the central bulge, suggesting a population of younger stars in that region. The lack of strong features indicates it is likely an older and more quiescent galaxy. The smoothness of the galactic structure suggests that it is not currently undergoing major interactions or mergers. The light is moderately redshifted, suggesting that it is not very far away.
