The object presents as a spiral galaxy, viewed at a significant angle relative to its plane. A distinct central bulge dominates the galaxy's structure, appearing nearly spherical and exhibiting a yellowish-white hue. The disk is visible, showing a subtle spiral structure. The arms are not sharply defined but rather appear as diffuse extensions from the central bulge. Color gradients across the disk suggest varying stellar populations, with bluer regions perhaps indicating ongoing star formation, particularly in the outer arms. The galaxy appears relatively isolated, with no obvious signs of major mergers or tidal disturbances. A slight asymmetry in the disk's shape may hint at a minor interaction or past merger event. The overall morphology suggests a galaxy in a relatively quiescent state of evolution.
