The galaxy presents as an elongated, edge-on spiral. A distinct, rounded bulge is visible at its center, characterized by a concentrated, yellowish-orange hue indicating an older stellar population. The disk appears thin and highly inclined, with the fainter light suggesting the possible presence of dust lanes obscuring parts of the disk, though these are not clearly defined. The galaxy exhibits a smooth overall appearance, with no obvious signs of recent major merger activity or strong tidal disturbances, though there may be some minor irregularities within the disk. The morphology suggests a relatively evolved system, exhibiting characteristics consistent with a substantial stellar mass and low star formation.
