The galaxy presents as a face-on or nearly face-on spiral galaxy, exhibiting a moderate central bulge. Spiral arm structure is visible, though somewhat flocculent and not sharply defined. A faint bar feature may be present, but its presence is not definitive. The galaxy displays a general blue hue, indicative of ongoing star formation. The bulge region appears more yellow/white compared to the arms, which likely indicates the presence of an older stellar population. There is some evidence of minor morphological disturbance or interaction, but it is not clear. Overall the galaxy appears to be of intermediate mass, with moderate star formation.
