The galaxy presents as a barred spiral, observed at an inclined angle to our line of sight. The central bulge appears prominent, displaying a yellowish hue indicative of an older stellar population. Two distinct spiral arms emanate from the ends of a faint bar structure, displaying a tightly wound morphology. These arms exhibit a bluer color, suggesting active star formation regions. The disk component is relatively smooth, with a light scattering and obscuring dust lanes. The galaxy's overall shape is elliptical, with a moderate axis ratio. There is no visible evidence of major mergers or tidal disturbances affecting the overall structure of this galaxy.
