The galaxy presents a relatively smooth morphology, appearing as a flattened, elongated structure. The central region exhibits a concentration of light with a yellowish hue, possibly indicating an older stellar population. The outer regions of the galaxy appear bluer, suggesting the presence of younger, hotter stars and potential star formation. There's a subtle asymmetry in the galaxy's shape. While the galaxy appears primarily undisturbed, there may be a minor tidal disturbance or interaction visible as a slight extension of the galactic disk on one side, possibly indicating a past or ongoing interaction with a smaller companion galaxy.
