The galaxy presents as an elongated, spindle-shaped structure, consistent with an edge-on or highly inclined disk galaxy. A central bulge is present, appearing as a bright, concentrated region. The disk shows a gradient in color, with bluer hues dominating the outer regions and a shift towards redder tones closer to the bulge. This color gradient likely indicates ongoing star formation in the outer regions of the disk, with older stellar populations concentrated in the bulge. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions, though some minor irregularities in the disk's light distribution may be suggestive of minor disturbances. The galaxy appears relatively smooth overall, but there are some hints of structures or features that could be spiral arms.
