The galaxy presents as a spiral type, exhibiting a well-defined disk structure. The spiral arms are clearly visible, though somewhat patchy in appearance, suggesting areas of active star formation interspersed with regions of lower stellar density. These arms emanate from a central bulge which appears moderate in size, not overwhelmingly dominant within the galaxy's overall structure. The bulge exhibits a yellowish-white color, indicative of an older stellar population.

The disk component shows a bluer hue, particularly noticeable along the spiral arms, implying the presence of younger, hotter stars. The overall color gradients suggest ongoing star formation within the disk. The galaxy's orientation is close to face-on, allowing a relatively unobstructed view of the spiral structure. There is no immediately apparent evidence of strong tidal distortions or ongoing major merger activity. Faint indications of a possible bar feature can be observed. 
