The galaxy presents as a slightly elongated, disk-like structure. Its color profile reveals a central region with a relatively bright and concentrated core, exhibiting a pink to magenta hue. This suggests a region of active star formation or potentially an active galactic nucleus. Extending outward from the core, a faint disk is visible. The color transitions towards blue-green, indicating the presence of younger stars and ongoing star formation activity within the spiral arms or disk features. There is some evidence of minor disturbance or asymmetry in the outer regions of the disk, potentially suggesting a past interaction or minor merger event. Overall, the galaxy appears to be relatively compact and moderately active in terms of star formation.
