This galaxy appears to be a spiral type, exhibiting prominent, well-defined spiral arms. These arms appear somewhat patchy with varying densities. There is evidence of active star formation within these arms. The bulge is not particularly large, and it does not dominate the galaxy's overall appearance. The galaxy lacks a strong central bar structure, with only a weak bar feature visible. No signs of major merging or significant tidal disturbances are immediately apparent. The galaxy is relatively bright, indicating a notable luminosity.
