The galaxy presents as a slightly inclined spiral, though its structure is somewhat diffuse. A central bulge is apparent, exhibiting a yellowish hue, possibly indicative of an older stellar population. The surrounding disk appears more mottled and bluish in places, suggesting the presence of regions of active star formation. Faint arm-like structures are discernible, though they are not sharply defined. The overall morphology suggests the possibility of a minor gravitational interaction or disturbance, as the disk appears slightly asymmetrical.
