The galaxy presents as a slightly elongated, cigar-shaped structure with a bright, concentrated central bulge. The disk component appears relatively smooth, suggesting a later-type spiral or lenticular morphology. A slight color gradient is visible, with the central bulge exhibiting a yellowish-white hue, potentially indicating an older stellar population. The outer disk regions appear somewhat bluer, which may imply the presence of ongoing or recent star formation. There is a hint of a minor disturbance in the disk, but overall, the galaxy appears relatively undisturbed. 
