The galaxy presents as a spiral type, with a moderate inclination relative to our line of sight. Two prominent spiral arms are visible, exhibiting a moderately wound structure. The arms display an uneven texture, suggesting regions of active star formation or dust obscuration. A central bulge is observable, with a size that is neither dominant nor insignificant relative to the disk. The bulge appears relatively smooth and concentrated. The disk exhibits a general bluer color than the bulge. There is no apparent strong bar structure bisecting the bulge. The overall morphology suggests a galaxy that is not currently undergoing a major merger, though there appears to be some distortion in its form.
