The galaxy presents a predominantly disk-like morphology, oriented at an inclined angle relative to our line of sight. Two distinct spiral arms are readily discernible, exhibiting a loose winding pattern. A bar-like structure appears to traverse the central region of the galaxy, showing a moderate strength. The central bulge shows intermediate characteristics, appearing neither overly dominant nor completely absent, and contributes noticeably to the overall luminosity. The disk displays a mottled texture with subtle color variations, hinting at regions of active star formation and varying stellar populations. There appears to be no significant evidence of a major ongoing merger or significant tidal disturbances.
