The galaxy presents as an edge-on spiral with a prominent, bright central bulge. The bulge appears yellowish, possibly indicating an older stellar population and reduced star formation within that region. The disk component of the galaxy is elongated and appears relatively smooth with less distinct spiral arm structure. The disk exhibits a bluer color than the central bulge, suggesting younger, hotter stars and ongoing star formation. There is little evidence of significant dust lanes within the disk. No major morphological disturbances or signs of recent merger activity are immediately apparent. Overall, the galaxy appears as a relatively undisturbed, moderately inclined spiral system.
