This galaxy presents as a generally smooth, elongated structure, exhibiting a noticeable color gradient across its extent. The central region displays a concentrated luminosity, appearing yellowish-white, suggestive of an older stellar population and possibly a bulge component. Moving outward from the core, the galaxy transitions to a bluish hue, hinting at the presence of younger, hotter stars within the spiral arms or outer disk. The elongation suggests a disk-like structure viewed at an oblique angle, implying it is not a face-on spiral. There is no visually obvious presence of strong dust lanes or prominent star forming regions. The lack of distinct morphological disturbances or tidal features indicates the absence of recent major merger events.