The galaxy presents as a slightly inclined spiral, possibly of an earlier type, based on the significant bulge component and relatively faint, somewhat ill-defined spiral arms. The bulge region exhibits a yellowish-white hue, suggesting an older stellar population. The disk component displays bluer regions, particularly at the outer edges, indicative of more recent star formation. There's some evidence of tidal disruption and possibly a minor merger event. The overall morphology indicates a gravitationally interacting system.
