The galaxy presents as an elongated, disk-shaped object with a reddish hue dominating its central region. A subtle gradient of color is observed, transitioning from a slightly greener tint at the outer edges towards the redder core. This color variation may indicate differences in stellar populations and activity across the galaxy, where there could be older stars that give the galaxy its red hue and younger stars that give the galaxy its green hue.

The galaxy appears to be relatively smooth, lacking prominent spiral arms or other distinct features. This suggests it may be a lenticular or possibly an elliptical galaxy, viewed edge-on, where the presence of a disk is suggested by the overall flattened morphology. No signs of major mergers or significant tidal disturbances are apparent in this image, suggesting that the galaxy is currently undergoing relatively quiescent evolution.
