The galaxy appears to be an edge-on spiral with a prominent, centrally concentrated bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. A faint, flattened disk extends outward from the bulge, appearing relatively smooth and featureless. The disk is significantly elongated, with a major-to-minor axis ratio indicating a highly inclined viewing angle. The colors within the disk are suggestive of ongoing, though potentially subdued, star formation activity. There is little evidence of distinct spiral arm structure in the visible light, likely due to the edge-on orientation obscuring detailed features. Overall, the galaxy seems to be a well-defined system with a classical bulge and disk morphology, observed at a high inclination angle.