The galaxy appears to be a spiral type, presenting a largely face-on orientation. Faint, loosely wound spiral arms are visible, emanating from a central, moderately sized bulge. The arms display a mottled texture with varying degrees of brightness suggestive of both active and passive star forming regions. There seems to be a slight asymmetry to the spiral structure, possibly resulting from a minor gravitational disturbance. The central bulge is fairly concentrated, exhibiting a yellowish hue, indicative of an older stellar population. Overall, the galaxy presents a fairly low surface brightness with a soft, diffuse halo. There is no clear evidence of a strong bar structure present within the galactic disc.
