The galaxy presents as a spiral, observed at a notable inclination to our line of sight. Spiral arms are readily apparent, exhibiting a relatively tight winding. The central bulge appears prominent, exhibiting a moderate size relative to the galactic disk. There is some evidence of a bar structure bisecting the bulge. The overall color profile suggests ongoing star formation, particularly within the spiral arms where bluer hues are concentrated. There is no significant sign of any interaction or merging event taking place with neighboring galaxies, no major disturbance is seen. The galaxy's features appear consistent with a classification as a spiral galaxy of intermediate luminosity.
