The galaxy presents as a disk galaxy, likely spiral, observed at an oblique angle. The disk exhibits a mottled texture, with regions of varying color and brightness suggestive of active star formation. The spiral arms appear tightly wound. The central bulge is prominent, exhibiting a bright, concentrated luminosity, transitioning smoothly into the disk. The galaxy shows no clear signs of major mergers or strong tidal disturbances, however there is a suggestion of minor asymmetry, perhaps indicating a smaller interaction. The overall color suggests a relatively high star formation rate, with a possible abundance of young, hot stars. The presence of neutral hydrogen is detected, in addition there are hints of ionized gas. The inner region of the galactic disk seems somewhat obscured or dusty.
