The galaxy presents as a spiral type, viewed at an angle oblique to face-on. A central bulge is visible, exhibiting a moderate size relative to the overall galactic disk. The bulge appears centrally concentrated with a yellow hue indicative of an older stellar population. The disk component shows distinct spiral arm structures emanating from the central bulge region. These arms are loosely wound and can be traced across a substantial portion of the galaxy's diameter. The arm morphology suggests a two-armed spiral pattern. Evidence suggests that this galaxy has a bar structure, however, it is difficult to tell if it is weak or strong based on the resolution of the data. The arms display a mottled appearance, likely from a mixture of HII regions and dust lanes. There also appears to be some interaction or disturbance occurring. It may be undergoing a minor disturbance or a more significant merger event, evidenced by asymmetries in the spiral arm structure or tidal features.
