The galaxy appears to be a spiral galaxy, exhibiting a relatively well-defined disk structure. Two prominent spiral arms are visible, tracing a moderate winding pattern outward from the central region. The arms are somewhat patchy, suggesting regions of active star formation. A central bulge is present, though not overwhelmingly dominant, contributing a significant portion of the galaxy's overall light. Evidence of a weak bar may be present, elongating the central region, although it is not pronounced. The galaxy is relatively face-on, allowing for clear observation of its spiral structure. The galaxy exhibits a bluer hue in the outer regions of its disk, transitioning to a yellower color toward its center.