The object presents as a spiral galaxy, observed at a near face-on orientation relative to our line of sight. The spiral structure is prominent, with two distinct arms emanating from the central region. These arms exhibit a moderate winding, neither tightly wound nor particularly loose. A strong bar structure is evident, bisecting the central bulge region. The bulge appears to be moderate in size, not overwhelmingly dominant but still substantial. There is no obvious indication of ongoing major mergers, though there appears to be some minor morphological disturbance within the disk, suggesting possible past interactions. The disk component of the galaxy contributes to the overall light profile.
