The galaxy presents as a disk galaxy, observed at a relatively high inclination. A prominent central bulge is visible, exhibiting a yellowish-orange hue suggestive of an older stellar population. The disk component displays a bluer color, particularly towards the edges, indicating the presence of younger, hotter stars associated with ongoing star formation. The overall form appears relatively undisturbed, though a slight asymmetry is noticeable, perhaps indicating a minor interaction or internal dynamics.
