The galaxy presents as a moderately inclined spiral or lenticular galaxy. A bright, concentrated central bulge dominates the core region, exhibiting a smooth, seemingly featureless profile. The outer disk displays a bluer hue, suggesting the presence of younger stellar populations and potentially ongoing star formation. The disk appears somewhat disturbed or asymmetric, as if experiencing a minor interaction or recent merger event. The galaxy's overall shape is elongated, which supports the high edge-on viewing angle. Some faint indications of spiral structure are visible, though not distinctly defined.
