The galaxy presents as a spiral, displaying a disk-like structure with moderate inclination to our line of sight. Two distinct spiral arms appear to emanate from the central bulge. The arms are relatively open, indicating loose winding. The nucleus exhibits a bright, concentrated glow indicative of an active galactic nucleus or a region of intense star formation within the bulge. The central bulge is a substantial fraction of the galaxy's overall size. The disk shows variation in color, suggesting differing stellar populations or dust distribution throughout the galaxy. There is no indication of significant tidal disturbances or ongoing major merger events. There appears to be a possible bar structure within the disk of the galaxy.
