The galaxy appears to be a spiral galaxy, viewed at a moderate inclination. It exhibits distinct spiral arm structures that are prominent. The central bulge is of small proportion relative to the overall galaxy size. A bar structure is also visible, spanning a considerable portion of the galaxy's diameter. There are no obvious signs of major merging activity or strong tidal distortions, though minor disturbances may be present. The galaxy's color suggests a mixed stellar population with both older, redder stars and regions of active star formation, indicated by bluer hues in the spiral arms. Overall, the galaxy presents a well-defined, relatively undisturbed spiral morphology.
