The galaxy presents as a well-defined, elongated structure, consistent with a disk galaxy viewed nearly edge-on. The central region exhibits a concentrated luminosity, suggestive of a prominent bulge component with an apparent rounded morphology. The disk appears relatively smooth, displaying minimal evidence of distinct spiral arm structures or substantial star-forming regions. Faint blue hues can be observed towards the outer edges of the disk, potentially indicative of younger stellar populations or ongoing, but subdued, star formation. There is no evident signs of major mergers or tidal disturbances affecting the overall morphology.
