The galaxy appears to be a somewhat elliptical, disk-like system. There's a bright, concentrated central bulge region exhibiting a bluish-white hue, which suggests a significant population of younger, hotter stars in that area. The surrounding disk shows a slightly redder color, indicating the presence of older stellar populations or dust absorption. The disk is not perfectly smooth; some subtle irregularities can be observed. There seems to be some possible evidence of a minor disturbance or interaction, as indicated by a slight asymmetry in the disk structure on one side. Overall, the galaxy does not show signs of major merging activity but may have undergone minor interactions in its past. A smooth morphology contributes a large portion of its overall classification, but definite features exist in the disk region. 
