The galaxy presents as a spiral, viewed at a moderate inclination angle. The central bulge appears prominent, displaying a yellowish hue. While a definitive bar structure is not immediately apparent, there is a slight elongation of the central region which may indicate the presence of a weak bar. Distinct spiral arms emanate from the central region. The arms are relatively tightly wound and exhibit some patchiness, possibly indicating regions of active star formation. The overall color gradient suggests a population of older stars concentrated in the bulge, with younger, bluer stars residing within the spiral arms. No major morphological disturbances or tidal features are immediately obvious, suggesting a relatively undisturbed evolutionary history.
